The galaxy presents as a lenticular or early-type spiral galaxy, seen nearly edge-on. It exhibits a prominent central bulge that appears relatively smooth and featureless in this image. A faint disk is discernible extending outwards from the bulge. There is some subtle structuring within the disk suggesting the possibility of spiral arms, but the low inclination makes definitive identification difficult. The galaxy displays a relatively red color profile overall, hinting at an older stellar population and reduced levels of current star formation. There is no clear evidence of ongoing merging activity or major tidal disturbances, although a slight asymmetry in the disk cannot be ruled out. The overall morphology suggests the galaxy is well settled.
