The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that dominates the overall luminosity. The color profile suggests a population of older stars, with a noticeable redder hue concentrated towards the core. There appears to be only minimal evidence of spiral arms or significant dust lanes. The overall structure shows a slight deviation from perfect circularity, hinting at possible minor gravitational interactions or internal dynamical processes. A small disturbed feature can be observed, suggesting some sort of minor disturbance within the galaxy.
