The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that appears nearly spherical. There is evidence of a slight disk-like component, though it is not well-defined. The color profile suggests a population of older stars, leaning towards redder hues, particularly within the core region. Hints of bluer colors exist in the surrounding areas, which might indicate recent, low-level star formation, though at a low rate. The galaxy does not obviously appear to be undergoing any major mergers or significant tidal interactions, but there is a slight asymmetry in its morphology, potentially indicating a past interaction.
