The galaxy presents a generally smooth, elliptical morphology. There is a slight elongation in the shape, but it is largely rounded. The primary body of the galaxy exhibits a concentrated, centrally bright structure, with a gradual decrease in luminosity towards the outer regions. The color profile indicates a redder overall hue, suggestive of an older stellar population. There are some indications of disturbances in the light profile, possibly indicating minor ongoing or past interactions. A potential merging event may be occuring, given the visual irregularity in its shape. Overall the galaxy seems to be in a late stage of its evolution.
