The galaxy presents a largely smooth, elliptical morphology with a high degree of central concentration. A bright, unresolved core region suggests the presence of a supermassive black hole or a dense population of stars. The galaxy exhibits a color gradient, transitioning from a bluer hue in the central regions to a redder tone in the outer halo. The absence of prominent spiral arms or dust lanes suggests that the galaxy is an early-type galaxy, likely an elliptical. There is no apparent evidence of any major ongoing merger activity or strong tidal features. Faint extended halo with some signs of disturbance or minor interactions. The galaxy appears relatively isolated within its immediate environment.
