The galaxy appears to be a relatively smooth, elliptical-type galaxy at a considerable distance, as evidenced by its small angular size. The main body presents a centrally concentrated luminosity profile, suggesting an older stellar population and a lack of significant ongoing star formation in the nuclear region.

The galaxy exhibits a slightly elongated morphology, deviating from perfect circularity. There is some indication of a potential minor disturbance in the galaxy's morphology on one side, possibly indicative of a recent minor merger event or tidal interaction, although this requires further investigation with higher resolution imaging and spectroscopic data. The primary color of the galaxy is consistent with the presence of both old and young stars.