The galaxy presents as a slightly elongated, lenticular-like structure. It exhibits a central bulge that appears largely smooth and featureless, with a bright, concentrated core. The light emitted from the galaxy is heavily concentrated in the yellow-red spectrum with subtle blue-green hues towards the outer edges of the disk, potentially indicating the presence of an older stellar population throughout the galaxy, with slightly younger populations towards the edges. The overall form is dominated by the bulge with a hint of a disk, but no distinct spiral arms are visible. No prominent dust lanes or active star-forming regions are clearly discernable within the image. The morphology suggests a relatively evolved system, possibly in the transition phase between spiral and elliptical. The overall smooth appearance indicates that it is unlikely to be undergoing any major merger events. The galaxy appears to have a estimated size around 6 kpc. The absolute magnitude of this galaxy is estimated to be high, particularly in the Z band, indicating a large and luminous galaxy. The estimated stellar mass is very high. The estimated star formation rate is very low, and the specific star formation rate is extremely low, indicating it is a quiescent galaxy with virtually no current star formation.
