The galaxy exhibits a smooth, elliptical morphology. The light distribution appears centrally concentrated, with a gradual decrease in intensity towards the outer regions. The color profile suggests a dominant population of older stars, indicated by the yellowish hue. There is no discernable dust lane or spiral arm structure visible. The overall appearance is that of a relatively undisturbed system, not showing any significant signs of recent mergers or tidal interactions. The size appears relatively compact.
