The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars. The outer regions display a gradual decline in luminosity with similar color, indicative of a well-mixed stellar population. There is no apparent dust lane or spiral structure visible. The overall form implies an evolved system with minimal ongoing star formation and without strong interactions. The galaxy's shape is approximately round. There is no evidence of any major merger or tidal disturbances.
