The galaxy presents as a smooth, centrally concentrated elliptical, exhibiting a yellowish hue indicative of an older stellar population. The light profile appears consistent with a high Sersic index, suggesting a dense, spheroidal structure. The ellipticity is noticeable, but not extreme, with the major axis oriented approximately horizontally in the image frame. There are no apparent spiral arm features or prominent dust lanes visible. The galaxy appears relatively isolated, with no nearby companions or signs of recent major mergers. The overall morphology suggests a relaxed system that has undergone significant dynamical evolution.