The galaxy appears as a smooth, elliptical-like object with a concentrated central bulge. It has a generally round morphology, with a slight elongation that could indicate some minor shaping or internal structure. The galaxy exhibits a yellowish-orange color, suggesting a population of older stars and a relatively low rate of ongoing star formation. There is no noticeable disk structure or spiral arm features; it appears largely featureless. The light distribution within the galaxy is relatively even, with a gradual decrease in brightness from the center outwards, however, there are some regions that seem to have different concentrations of density. The overall appearance suggests a massive galaxy that has undergone significant stellar evolution. There is no evidence of any major mergers or tidal disturbances.
