The galaxy presents a generally smooth morphology, exhibiting a bright central region that is nearly spheroidal in shape. There is a slight indication of possible disk structure. The color is dominated by yellowish and reddish hues, which implies an older stellar population and lower ongoing star formation. The overall appearance suggests a galaxy with a significant bulge component, and potentially a fainter, diffuse disk. There might be some subtle disturbances in the overall structure, perhaps indicative of minor tidal interactions or internal instabilities.
