The galaxy appears to be a relatively smooth, elliptical type. Its core is a bright, concentrated region, suggesting a high density of stars. Moving outward from the core, the light gradually diminishes, forming a diffuse halo. There is a slight elongation in the galaxy's shape, tending toward a cigar-like morphology. No distinct spiral arms or significant dust lanes are discernible within the galaxy's structure. Faint color gradients are observed, possibly indicating variations in stellar populations or metallicities across the galaxy. The galaxy appears relatively isolated and does not seem to be undergoing a major merger or tidal disruption. Minor disturbances cannot be ruled out.