The galaxy presents an elliptical morphology, appearing largely smooth and rounded. It exhibits a centrally concentrated brightness profile, with the luminosity gradually decreasing outwards from the core. The galaxy displays subtle color gradients, transitioning from a slightly bluer hue in the central regions to a more reddish tint in the outer halo, suggesting possible variations in stellar populations or dust content. There is no evidence of distinct spiral arms or a prominent disk structure. The overall appearance indicates a relatively evolved system with a likely older stellar population. Close inspection does not reveal signs of major ongoing mergers or significant tidal disturbances, although a subtle asymmetry may indicate a past minor interaction.
