The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that graduates into a fainter, less defined outer halo. The overall color profile suggests a population dominated by older stars, with a subtle reddish-yellow hue concentrated towards the center. No prominent dust lanes or spiral arm structures are discernible; the morphology is largely featureless. There may be minimal, minor disturbances possibly indicating gravitational interaction. The galaxy appears relatively isolated. Its smooth and rounded appearance suggests that it is an early-type galaxy.
