The galaxy presents as a centrally concentrated elliptical or S0-type morphology. There's a dominant, smooth bulge that comprises the majority of the galaxy's light. The color profile indicates a redder hue throughout, suggesting a population of older stars and a low dust content. The galaxy appears relatively undisturbed, exhibiting no prominent tidal features or signs of recent major mergers. It is moderately luminous and relatively compact, presenting a fairly symmetric profile without any substantial spiral arm structure visible. The light is fairly diffused in the outer regions of the galaxy, with a high degree of central concentration. There may be some subtle evidence of minor asymmetry in the outer regions, potentially indicative of a past interaction or merger event.
