The galaxy presents a largely smooth, elliptical morphology. The core region exhibits a concentrated, bright luminosity, appearing almost spherical in shape. A subtle color gradient is observed, shifting from a yellow-orange hue in the central region to a slightly bluer tint in the outer halo. This halo displays a gradual fade in intensity with increasing distance from the core, suggesting a decreasing stellar density. A possible minor disturbance or tidal feature is visible as a faint extension or plume emanating from one side of the galaxy, indicating a potential past interaction or ongoing accretion event. Overall, the galaxy appears relatively isolated with no other interacting galaxies in close proximity.
