The galaxy presents as a relatively smooth, elliptical-like structure, elongated with a moderate aspect ratio. The central region exhibits a concentrated luminosity, appearing brighter than the outer regions. There is some apparent color variation across the galaxy, with a reddish hue more prominent in the central region and a greenish tint visible in the periphery, potentially indicating differing stellar populations or dust distribution. No distinct spiral arms or bar features are discernible. There is no obvious sign of any major ongoing merger activity or strong tidal disturbances, though subtle asymmetries might suggest minor interactions.
