The galaxy presents as a centrally concentrated system with a largely smooth and rounded morphology, suggestive of an elliptical or S0 type. The central region exhibits a bright, compact core, likely indicative of an actively star-forming region or an active galactic nucleus. A faint, diffuse halo surrounds the core, gradually fading into the background sky. There is a slight elongation to the overall shape but is mostly spherical. There is little to no evidence of spiral arm structure or significant dust lanes. The galaxy appears relatively undisturbed, with no clear signs of recent mergers or tidal interactions. Color gradients are subtle, with a slightly bluer hue in the outer regions, possibly indicating younger stellar populations.
