The galaxy presents a morphology that is largely smooth and elliptical in appearance. Its overall shape suggests a relatively high degree of sphericity, with a minor deviation towards a slightly elongated form. The galaxy exhibits a distinct color gradient, transitioning from a bluer hue in the outer regions to a more reddish tone towards the central bulge. This color variation may indicate a difference in stellar populations, with younger, bluer stars populating the periphery and older, redder stars concentrated in the core. There appears to be little to no evidence of spiral arm structures or significant dust lanes. Faint features suggest possible minor disturbances or tidal interactions, yet its overall structure remains largely undisturbed. The light appears to be centrally concentrated.
