The galaxy presents an elliptical morphology, exhibiting a smooth and somewhat diffuse structure. The central region is characterized by a bright, concentrated core, suggestive of a substantial stellar population and potentially a supermassive black hole. The galaxy displays a gradual decrease in surface brightness from the center outwards, with the outer regions appearing fainter and less defined. There's a subtle color gradient, transitioning from a yellowish-white core to a slightly bluer hue in the outer regions, which might indicate the presence of younger stars or ongoing star formation in the galactic outskirts, though at a low rate. There appears to be a slight asymmetry in the galaxy's overall shape, possibly indicating a past or ongoing minor interaction with another galaxy. However, no prominent tidal features or distortions are immediately apparent, which suggests that any interaction may have been relatively minor or occurred in the distant past. The galaxy is relatively compact, with a well-defined edge.
