This galaxy presents as a centrally concentrated elliptical, appearing largely smooth and featureless across its extent. The core region exhibits a yellowish hue, indicative of an older stellar population. Moving outward from the center, the galaxy displays a gradual transition to a bluer color, suggesting the presence of a younger, though less dominant, population of stars in the outer regions. The overall shape is roughly elliptical, with no apparent spiral arms or significant dust lanes visible. There appears to be a very slight, almost imperceptible, asymmetry in the outer isophotes, hinting at a possible minor interaction or past merger event, though this is difficult to ascertain definitively from the available image. The galaxy appears relatively isolated, with no immediately obvious signs of a major ongoing interaction or merger.
