The galaxy presents as an elliptical structure with a concentrated central bulge. There is no apparent spiral arm structure. Color gradients suggest a population of older stars dominating the bulge, indicated by the reddish-orange hue, while the surrounding disk appears slightly bluer, potentially indicating some ongoing star formation. The galaxy's overall morphology appears relatively smooth, but with subtle irregularities that could be indicative of minor disturbances or internal activity. It is difficult to ascertain the presence of a distinct dust lane based on the image resolution.
