This galaxy appears to be relatively compact with an elliptical morphology. It exhibits a bright, concentrated core that transitions into a more diffuse halo or envelope. The color profile suggests a mixture of stellar populations; the central region displays a bluer hue, which may indicate the presence of younger, hotter stars, while the outer regions shift towards a slightly redder tone, implying older, cooler stars.

There's a hint of asymmetry in the outer halo. A disturbance is present that may indicate a possible minor merger event. The overall structure appears relatively smooth with very little apparent substructure.
