The galaxy presents a primarily smooth morphology, exhibiting a concentrated central bulge which radiates strongly. The overall color profile suggests a relatively old stellar population, with light shifted towards the redder end of the spectrum. There is faint, but discernible, evidence of a disk-like structure surrounding the central bulge, although the disk appears somewhat disturbed or irregular. Possible minor disturbances or tidal features may be present, suggesting a potential interaction or merger event in the galaxy's past. The galaxy appears to be generally elliptical but not perfectly rounded, slightly oblong, possibly due to the disturbances. The galaxy has a noticeable degree of star formation, even if in a subdued state.
