The galaxy presents as a single, relatively smooth object with minimal apparent substructure. The overall shape appears close to circular, with no obvious distortions suggestive of tidal interactions or recent merger events. The color is primarily yellowish-orange, indicating a population of older stars and a likely low rate of ongoing star formation. There is no clearly visible nucleus or central bulge, though the limited resolution prevents a definitive conclusion on the presence and morphology of a central structure. Overall, the galaxy appears to be an evolved system, likely an elliptical or lenticular type, with a dominant population of older stars and minimal current star formation activity. The estimated size is consistent with a galaxy of intermediate dimensions. Evidence for merging activity is low, suggesting a relatively isolated evolutionary history.
