The galaxy presents as a moderately elliptical object, its overall shape being close to circular, with an inclination that is somewhat face-on. The galaxy exhibits a smooth, centrally concentrated luminosity profile indicative of a single bulge-dominated system. There's a subtle color gradient with a slightly bluer hue at the edges that becomes progressively more yellow towards the center. This color variation hints at potentially varying stellar populations within the galaxy, suggesting a population of younger, bluer stars in the outer regions and a prevalence of older, redder stars in the galactic nucleus. No distinct spiral arm structures or dust lanes are discernible, further supporting its classification as an early-type galaxy. The galaxy appears to be relatively isolated, without any obvious signs of recent major merger events or significant tidal interactions.
