The galaxy presents as a slightly elongated, though predominantly smooth, distribution of light. It lacks any discernible spiral arm structure or prominent dust lanes, appearing featureless across the observed wavelengths. The morphology suggests a possible elliptical or lenticular classification. The color is slightly reddish-yellow, which is consistent with an older stellar population and less ongoing star formation. The apparent size is small, indicating a significant distance or an intrinsically compact object. There are hints of tidal disturbances, which may suggest the presence of some kind of external forces acting on this galaxy. Overall, the galaxy appears to be a relatively evolved system, potentially transitioning from a more active phase to a quiescent state.
