The galaxy presents as a largely smooth, elliptical structure. It exhibits a noticeable elongation, appearing cigar-shaped. The light profile is concentrated towards the center, displaying a bright, diffuse core. Moving outward from the core, the light gradually fades into the surrounding space. There are subtle color variations across the galaxy; the core region appears slightly more yellow/red, while the outer regions show hints of blue, suggesting possible variations in stellar populations or dust content. The galaxy lacks any distinct spiral arm structure or prominent dust lanes, supporting its classification as an elliptical galaxy. There are no signs of ongoing major merger activity, though minor disturbances cannot be entirely ruled out at this resolution.
