The galaxy presents as an elliptical or lenticular type with a largely smooth morphology. The overall color index suggests a relatively evolved stellar population. There is a slight elongation visible in the galaxy's shape, although it is mostly round, possibly indicating a minimal amount of rotational support. No strong signs of recent or ongoing merger activity are apparent, but there is a slight asymmetry in the galaxy's outer regions that could suggest some form of minor interaction in the past. The galaxy exhibits a concentrated core with a gradual decrease in luminosity towards its outer edges.
