The galaxy appears to be relatively bright, exhibiting a centrally concentrated luminosity profile. The morphology is largely smooth and spheroidal in appearance, suggesting an elliptical or S0 classification. However, the presence of some subtle irregularities in the outer regions indicates it may have some features. The galaxy's color is generally redder in the core and appears to become slightly bluer in the outer regions. This color gradient could imply older stellar populations dominating the core, with younger, bluer stars potentially present in the outer regions or faint disk-like structure. There is the suggestion of a minor disturbance, possibly related to a past or ongoing minor merger event. There may be slight asymmetries in the isophotes or a very faint tidal tail, but these features are subtle.
