The galaxy presents as a relatively smooth object with a round morphology. It exhibits a concentrated luminosity profile, suggesting an elliptical or lenticular classification. The color appears to be reddish-yellow, indicative of an older stellar population with lower levels of ongoing star formation. No distinct spiral arms or prominent dust lanes are discernible, further supporting the notion of a passively evolving system. There is a chance of a companion galaxy nearby that is visually distinct from the primary object. The light appears to be relatively undisturbed, with no signs of a strong tidal interaction or recent merger. Overall, the observed features point towards a galaxy with a significant spheroidal component and suppressed star formation activity.
