The galaxy presents as an elliptical structure with a smooth appearance and a moderately concentrated central bulge. There is a slight elongation to the galaxy's shape, deviating from perfectly round. Faint, diffuse extensions or potential tidal features may be present, indicating a possible history of interaction or disturbance. The light distribution is relatively even across the galaxy's body. The overall color is consistent with an older stellar population. There might be a region of more intense star formation. There does not appear to be a distinct disk. There are no strong indicators of an on-going major merger, but minor distortions are present. 
