The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a somewhat elliptical morphology, appearing neither perfectly spherical nor highly elongated. The core region displays a yellowish-white hue, suggestive of an older stellar population. Moving outwards from the center, a slight bluish tinge becomes apparent, potentially indicating the presence of younger, hotter stars within a faint disk-like structure. There is no obvious spiral arm structure or prominent dust lanes visible. Only minor disturbances are seen in the galaxy. The galaxy appears to be relatively isolated, with no immediately apparent signs of tidal interactions or major mergers, even though minor mergers cannot be ruled out.
