The galaxy presents a largely smooth and concentrated morphology, exhibiting a primarily elliptical structure. It appears relatively rounded, with a slight elongation discernable along its major axis. The light distribution is centrally concentrated, with a gradual decrease in intensity moving outwards from the core. The galaxy exhibits a color gradient, transitioning from a yellowish hue at the core to a slightly redder tint in the outer regions. There is no visible evidence of spiral arms or significant dust lanes within the galaxy's structure. No signs of major mergers or tidal disturbances are observed in its immediate vicinity. The galaxy appears relatively isolated and undisturbed in its current environment.
