The galaxy presents as a largely featureless, elliptical morphology. Its luminosity profile appears centrally concentrated, with a smooth, gradual decline in surface brightness extending outward from the core. The dominant color is a yellowish-white hue, suggestive of an older stellar population, with little evidence of ongoing star formation. The overall structure suggests minimal signs of recent mergers or tidal disturbances. The galaxy exhibits a relatively round shape, lacking any prominent disc-like or spiral arm structures. There may be a very slight deviation from perfect ellipticity, hinting at a minor interaction in the past.
