The galaxy presents a generally smooth, elliptical morphology. The light distribution shows a concentration towards the center, indicating a possible bulge component. There is a slight elongation of the galaxy, with the major axis appearing to be oriented horizontally in the image. The color gradient appears relatively consistent across the galaxy, suggesting a lack of significant dust lanes or prominent star-forming regions. No obvious signs of tidal tails or significant distortions are apparent, implying no major recent mergers or interactions. The galaxy exhibits a diffuse halo, with its light gradually fading into the background sky.
