The galaxy presents as a relatively compact object with a discernible, though not sharply defined, elliptical morphology. The central region exhibits a high surface brightness, appearing as a bright, diffuse core. Proceeding outwards, the light gradually diminishes without distinct spiral arm features. A slight asymmetry is visible in the outer regions, possibly indicative of minor tidal disturbances or interactions. Overall the galaxy appears to be relatively smooth in texture. Its color suggests a population of stars with intermediate ages. The estimated effective radius of the galaxy is approximately 6.7 kpc.
