The galaxy presents a generally smooth appearance, with a dominant central bulge. Its shape appears largely spheroidal, transitioning from a bright, concentrated core to a diffuse halo. There is little evidence of spiral arm structure or distinct disk features. The color gradient indicates a population of older stars. The overall morphology suggests an elliptical galaxy, possibly of type E3-E5 given its apparent ellipticity. There is very little indication of ongoing merging activity, but I cannot rule out a minor disturbance.
