The galaxy presents a smooth, rounded morphology, indicative of an elliptical or lenticular type. There is a clear central concentration of light, suggesting a prominent galactic nucleus. A subtle color gradient is observed, transitioning from a reddish hue at the core to a slightly greenish-yellow periphery. This could be due to a population of older stars concentrated towards the center, with younger star formation occurring in the outer regions, although at a low rate. There is no apparent spiral structure or significant dust lane obscuration, suggesting a lack of ongoing major mergers or disk features. The galaxy appears relatively undisturbed, with no signs of tidal tails or strong gravitational interactions, based on its observed morphology. The general appearance points toward a relatively evolved system.
