The galaxy appears to be an elliptical type, with a smooth, featureless morphology. It exhibits a centrally concentrated luminosity profile, with a bright, dense core that gradually fades outwards into a more diffuse halo. The overall shape of the galaxy is roughly circular. There is a subtle color gradient visible, shifting from a slightly bluer hue in the outer regions to a more yellow/orange core. There is no evidence of spiral arms, dust lanes, or any significant tidal disturbances to suggest recent merging activity. The absence of any clear features suggests a relatively evolved system, dominated by older stellar populations.
