The galaxy presents as a dominant, centrally located object with a smooth, elliptical morphology. It is a relatively round structure with a slight elongation that is difficult to discern given the image quality. There does not appear to be any distinct disk component, spiral arms or prominent dust lanes, indicating it is likely an early-type galaxy. No major disturbances due to mergers or tidal interactions are visibly apparent, although some minor asymmetrical features might be present in the outer regions upon further inspection. The galaxy exhibits a color profile consistent with a population of older stars, displaying a reddish-yellow hue. There is no evidence of ongoing or recent star formation in the galaxy's core or outer regions within the limits of this data.
