The galaxy presents an elliptical morphology, displaying a smooth, centrally concentrated light profile. A prominent bulge dominates the structure, exhibiting a yellowish-white hue, suggestive of an older stellar population. The overall color gradient indicates a potential lack of significant recent star formation activity within the primary body. The outer regions appear fainter and less defined, possibly indicating a gradual decline in stellar density. There is a faint suggestion of a minor disturbance or extended feature located to one side of the galaxy, though the resolution limits a precise assessment. The galaxy appears relatively isolated, with no immediately obvious signs of major mergers or interactions.
