The galaxy exhibits a generally elliptical morphology, appearing mostly smooth with a concentrated central bulge. It presents a relatively round shape, showing little or no distinct disk structure or spiral arms in the visible wavelengths. The color profile suggests a population of older stars, exhibiting a yellowish-white hue overall. The galaxy does not display any obvious signs of ongoing major mergers or significant tidal disturbances. While some minor irregularities are subtly visible within the surrounding galactic halo, this does not appear to be overly dramatic. The central core of the galaxy appears as the brightest region, gradually fading outwards. The small angular size indicates that it is a considerable distance away. The light suggests moderate star formation activity.
