The galaxy presents as a centrally concentrated system with a smooth morphology. The core region exhibits a distinct yellowish-orange hue, suggesting an older stellar population, potentially dominated by evolved stars. The overall shape is elliptical, though deviates slightly from perfect circularity. There is a subtle gradient in color and intensity from the core towards the outer regions. The outer regions appear fainter and possess a slightly bluer tint, possibly indicating the presence of some younger stars, though the galaxy is dominated by older stars. No distinct spiral arms or prominent dust lanes are visible. There is a very slight indication of a possible minor tidal disturbance but the galaxy appears to have an undisturbed shape. Overall, this galaxy appears to be a relatively massive, evolved system with little ongoing star formation.
