The galaxy presents as an elliptical or lenticular type. The light profile is generally smooth with a concentrated central bulge exhibiting a yellow-orange hue, potentially indicating an older stellar population. Fainter, bluer light extends from the center, suggesting the presence of some star formation activity, albeit relatively weak. The overall shape is elongated, cigar-like, but with a slight roundness, not perfectly linear. There are no apparent signs of major tidal disturbances or ongoing merging activity; it appears relatively undisturbed. Its color index suggests it is a mature galaxy with moderate mass and low specific star formation rate.
