The galaxy presents as an elliptical morphology, exhibiting a smooth, centrally concentrated light distribution.  The core appears bright and relatively featureless, transitioning gradually to a fainter, diffuse halo. Color gradients suggest a population of older stars dominating the central regions, shifting to slightly bluer populations in the outer halo.  The axial ratio is close to one, indicating a near-circular appearance. No prominent spiral arms or dust lanes are discernible. There is no obvious evidence of tidal features or interaction with other galaxies.
