The galaxy presents as a moderately bright, elliptical structure with a noticeable color gradient. The central region exhibits a concentrated, yellowish-white hue, suggesting a population of older stars. Moving outward from the core, the color shifts to a more diffuse, slightly bluer tone, possibly indicating younger stellar populations in the outer regions. The galaxy appears largely smooth, with minimal visible signs of spiral arms or distinct dust lanes. Its overall shape suggests a moderate degree of ellipticity, falling somewhere between a nearly circular and a cigar-shaped morphology. There are no obvious signs of ongoing major mergers or tidal disturbances, although a subtle asymmetry in the outer regions could hint at minor gravitational interactions or internal dynamical processes.
