The galaxy presents as an elliptical morphology with a smooth, diffuse light distribution. The central bulge appears bright and concentrated, with a yellow-white hue, suggesting a population of older stars. The outer regions of the galaxy show a gradual decline in luminosity, fading into the background. There is a subtle color gradient, with the core appearing slightly redder than the outer regions. No distinct spiral arms or dust lanes are visible. There is a slight asymmetry. There is no obvious evidence of an ongoing merger event or significant tidal disturbances in the immediate vicinity. The galaxy appears relatively isolated and well-formed.
