The galaxy presents a largely smooth morphology, with a slight degree of ellipticity. The color profile shows a concentrated yellowish core, indicative of an older stellar population. Fainter blue hues are observed extending outward from the core, suggesting the presence of some younger, bluer stars, potentially within a faint disk-like component. There is no evidence of strong tidal features or ongoing major mergers; however, a slight asymmetry could indicate a minor interaction in the past. The object appears relatively undisturbed and quiescent.
