The galaxy presents as a relatively smooth structure, with a dominant central bulge that exhibits a concentrated luminosity gradient. There are subtle colour variations across the galaxy, with the core appearing slightly yellower than the outer regions, possibly indicating a difference in stellar populations or dust content. A faint, diffuse halo surrounds the central body, extending outwards and gradually fading into the background sky. The overall shape is somewhat rounded, though there are hints of a slight flattening which could indicate a disk component, but such components are not well resolved in the image. There is no strong evidence of spiral arms or significant dust lanes. The galaxy appears undisturbed, without obvious signs of a recent major merger or tidal interactions.
