The galaxy presents as an elliptical or lenticular type, appearing largely smooth with a concentrated central bulge. It displays a generally rounded morphology, with a slight elongation. A faint tidal feature or interacting companion is seen offset from the galaxy's core, suggesting a possible gravitational interaction. Color analysis reveals a dominant yellow-orange hue, suggestive of an older stellar population. The galaxy's overall luminosity indicates it is likely a massive system with little to no star formation. Evidence suggests a significant probability of merger activity in its recent history. 
