The galaxy presents as a moderately bright, elliptical or lenticular system. The light is centrally concentrated with a smooth, diffuse morphology. There is a slight elongation in the shape, suggesting a deviation from perfect circularity. A subtle color gradient is observed, with a whiter hue towards the galactic center, gradually transitioning to a bluer tinge in the outer regions. No distinct spiral arms or prominent dust lanes are visible. The overall appearance indicates an evolved stellar population, with signs of recent star formation. The system appears relatively undisturbed, showing no signs of major tidal interactions or ongoing mergers.
