The galaxy presents as a luminous, elongated object with a prominent central bulge. The light distribution is dominated by yellowish-orange hues, suggesting an older stellar population. The galaxy exhibits a smooth texture with no apparent spiral arm structure or distinct dust lanes, indicating it's likely an elliptical or lenticular galaxy. There is a hint of asymmetry in the outer regions, possibly indicative of a minor tidal interaction or past merger event. Overall, the galaxy appears to be relatively massive with a moderate star formation rate.
