The galaxy appears as a centrally concentrated, roughly elliptical object. It has a bright, yellowish core that gradually diffuses outward. The outer regions exhibit a fainter, more reddish-orange hue. The overall structure indicates a smooth profile, with no apparent spiral arm structures or significant dust lanes visible in this image. There is a slight asymmetry in the outer regions, potentially indicative of a minor gravitational disturbance or interaction. The galaxy appears relatively isolated, showing no signs of a major ongoing merger. The distribution of light suggests a relatively old stellar population, with a low rate of ongoing star formation.
