The galaxy presents as a relatively smooth, elliptical-like structure, with a concentrated central region. There is evidence of a possible slight disk-like feature. The color profile indicates a mix of stellar populations, with the central region displaying a yellowish-white hue, suggesting older stars. There are traces of green and blue, which may suggest ongoing or recent star formation. The galaxy appears to be relatively undisturbed, showing no signs of major mergers or significant tidal interactions. The overall morphology suggests an evolved system, possibly transitioning from a more active star-forming phase to a quiescent state.
