This galaxy presents as a relatively compact, elongated structure. The color profile suggests an older stellar population dominating its composition, particularly in the central region, where the light appears redder. The overall smoothness of the light distribution suggests a lack of significant spiral arm structure or active star formation regions. It's likely an elliptical galaxy, possibly with a slight central bulge. There is some indication of a subtle disk-like component, but it is not well-defined. There might be some minor disturbances in the galaxy's shape, but overall, it appears relatively undisturbed.
