This galaxy exhibits a generally smooth morphology, suggesting a possible elliptical or lenticular classification. The light distribution is highly concentrated toward the center, which indicates a prominent bulge. There may be some evidence of a very faint, diffuse disk surrounding the bulge, but the overall structure lacks strong spiral arm features. The galaxy appears more or less round, though there may be a slight elongation. There are no obvious signs of major mergers or significant tidal disturbances in its immediate vicinity. The color is consistent with a population of older stars.
