The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge region that appears to be the brightest component. The overall color profile suggests a population of older stars, with a yellowish to reddish hue dominating the galaxy's light. There is no clear evidence of spiral arms or significant dust lanes. The shape is observed to be mostly round, with only a slight elongation, although image resolution is limited. There are no indications of strong tidal disturbances or ongoing mergers. Star formation appears to be minimal based on color. The galaxy's apparent size is small, and the light is concentrated.
