The galaxy presents as a smooth, centrally concentrated object. It exhibits a roughly elliptical morphology with a high degree of circularity. No obvious spiral arms or bar structures are discernible. The light distribution appears relatively uniform and diffuse across the galactic body. The core region exhibits a yellowish hue, suggestive of an older stellar population, while the outer regions show a hint of bluer light, potentially indicating some low-level star formation. There is no visible evidence of major tidal disturbances, mergers, or significant dust lanes. The overall impression is that of a relatively undisturbed and evolved system.
