The galaxy presents a predominantly smooth morphology, with an elliptical appearance. The central region exhibits a bright, concentrated core, suggesting a high stellar density. Proceeding outwards, the luminosity gradually diminishes, forming a diffuse halo. The overall color profile indicates a population of older stars, as evidenced by the reddish-yellow hue, although some hints of bluer light are present in some areas, hinting at regions of younger stellar populations. There is no clear evidence of spiral arms or a distinct disk structure. There is little indication of active star formation in the galaxy, and no signs of tidal disturbances or ongoing mergers. The galaxy is generally isolated in the observed field.
