The galaxy presents as a moderately bright, elliptical or lenticular structure with a smooth, concentrated central bulge. The light profile suggests a relatively old stellar population, contributing to its yellowish hue, indicative of reduced ongoing star formation. There is a very faint presence of spiral arms, which might categorize it as a late stage spiral transitioning into a lenticular galaxy. The central bulge is compact and dominates the overall light emission. The galaxy appears mostly undisturbed with little to no evidence of tidal features, major mergers or active star formation, though a minor companion object appears to be nearby. The overall morphology suggests a relatively quiescent galaxy, past its peak star-forming phase.
