The galaxy presents as an elliptical or lenticular type with a smooth, concentrated central bulge. It exhibits a moderate degree of ellipticity. The overall color profile suggests an older stellar population, with a yellowish-white hue dominating the central region. There is a slight color gradient towards the outer regions, exhibiting a marginally bluer tint that may imply a low level of ongoing star formation. A region of redder emission to the Northwest seems associated with a region of recent star formation or tidal disruption. No obvious spiral arm structure is discernible. There appears to be some evidence of minor gravitational interaction or disturbance, suggested by an asymmetrical elongation, particularly towards the bottom of the image. The galaxy does not appear to be undergoing a major merger, but the possibility of minor tidal interactions or past accretion events cannot be ruled out.
