The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The color profile suggests a population of older stars, indicated by the yellowish hue, although bluer tones are visible. There is little evidence of spiral arms or significant dust lanes, lending further support to an early-type morphological classification. The galaxy appears fairly isolated, with no obvious signs of tidal interactions or ongoing mergers, and no major distortions or disruptions in its overall shape. There is some slight indication of disturbance in the outer edges of the galaxy, potentially suggesting a minor interaction. Based on the distribution of light, this galaxy may be of considerable mass, a fairly old elliptical galaxy.
