The galaxy appears as a roughly elliptical object with a concentrated central bulge. The light distribution suggests a smooth profile, potentially indicative of an older stellar population. The galaxy exhibits a yellow-orange hue, which implies the presence of evolved stars and a lack of significant recent star formation. There are no obvious spiral arms or prominent dust lanes visible. The shape is slightly elongated, and the orientation is non-edge-on, allowing for a partial view of its structure. The overall appearance is consistent with that of an elliptical galaxy or a lenticular galaxy with a dominant bulge. There may be some faint structure on the outer edges, however that cannot be confidently confirmed.
