The galaxy presents as a centrally concentrated object with a generally elliptical morphology. The central region is characterized by a bright, relatively smooth luminosity profile, exhibiting a yellowish-white hue. Moving outward from the core, the galaxy displays a gradual decrease in surface brightness. The outer regions exhibit hints of bluer concentrations, potentially indicative of regions of more recent or ongoing star formation, or of resolved stellar populations. The galaxy appears to be relatively undisturbed, showing no obvious signs of major mergers or tidal interactions. However, there are subtle asymmetries and disturbances present, suggesting minor disturbances. The overall shape is elongated, with the light distribution less extended along the minor axis. The galaxy's radial profile appears to be somewhere in between that of a spiral and an elliptical galaxy.
