The galaxy appears to be a relatively smooth, elliptical galaxy. Its morphology is predominantly spheroidal, lacking any obvious spiral arm structures or a prominent disk component. The light distribution is highly concentrated, with a bright central bulge that gradually fades towards the outer regions. There is no clear evidence of ongoing or recent major mergers or tidal disturbances, although minor asymmetries may be present. The galaxy exhibits a color gradient, becoming bluer towards the outer regions. This may indicate recent or ongoing star formation in these regions, contrasting with the older stellar populations expected in the central bulge. The overall color suggests a population of intermediate-age stars. The galaxy appears to be relatively massive, with a moderate rate of star formation.
