The galaxy presents a somewhat elliptical morphology, though some disk-like structure can be discerned. The central region exhibits a concentrated and bright intensity, suggesting a possible bulge. The colour appears to be generally redder suggesting an older stellar population. The smoothness of the galaxy is moderate and the colours suggest a galaxy undergoing little star formation. There is no obvious presence of strong tidal tails or distinct merger features. However, slight asymmetry hints at possible minor disturbances.
