The galaxy presents as an elliptical form, with a smooth, largely featureless structure. The luminosity profile increases towards the central region, suggesting a concentration of stars and potentially a central supermassive black hole. The galaxy exhibits a subtle elongation, appearing somewhere between round and cigar-shaped. No distinct spiral arms or bar structures are apparent. There are no prominent signs of ongoing mergers or significant tidal disturbances in the immediate vicinity. The color gradient transitions from a yellowish-white core to a more reddish hue in the outer regions, which may indicate an older stellar population dominating the periphery.
