The galaxy presents a generally smooth and rounded appearance, indicative of an elliptical morphology. The central region exhibits a bright, concentrated core, suggesting a high density of stars. There is a gradual decrease in luminosity moving outwards from the center, with no distinct spiral arm structure or significant dust lane features readily apparent. The galaxy appears relatively undisturbed, with no obvious signs of recent major mergers or tidal interactions. Color gradients suggest a population of older stars. The overall structure hints at a quiescent system with relatively low levels of on-going star formation.
