This galaxy presents as a moderately bright, elliptical form. The central bulge is prominent and appears relatively smooth with a concentrated luminosity. Progressing outwards from the bulge, the light intensity diminishes, indicating a possible gradual decrease in stellar density. The galaxy's shape can be approximated as an elongated spheroid. A slight warping or irregularity in the disk-like structure is observed, possibly suggestive of minor gravitational interaction or internal disturbances. The overall color is suggestive of an older stellar population, dominated by redder giants. There is a suggestion of a smaller companion galaxy or tidal tail on the bottom left.
