The galaxy presents as a singular, relatively smooth structure, exhibiting a concentrated central bulge that radiates prominently. The galaxy's overall shape appears largely elliptical, with minimal indication of spiral arms or significant disk features. There is a subtle color gradient observed, transitioning from a bright, yellowish core to a slightly bluer, albeit diffuse, outer halo. The galaxy seems undisturbed, displaying no apparent signs of ongoing mergers or significant tidal interactions. The light distribution suggests an older stellar population, particularly in the core, although some residual star formation may be present in the outer regions, contributing to the bluer hue.
