The galaxy presents as a predominantly smooth, elliptical object. It exhibits a somewhat spheroidal morphology, appearing largely rounded in shape. There is no obvious indication of spiral arm structure or a pronounced disk. The galaxy’s light profile appears to be smooth and diffuse, suggesting a well-mixed stellar population. Its color is relatively red, indicative of a population of older stars and a likely lack of significant ongoing star formation. There is no visually apparent evidence of a major ongoing merger or significant tidal disturbances, although the presence of minor disturbances cannot be ruled out with this image alone.
