The galaxy presents as a centrally concentrated elliptical, exhibiting a smooth, primarily featureless morphology. The core region displays a notably high surface brightness, indicating a significant stellar density. Progressing outward from the core, the luminosity gradually decreases, transitioning into a more diffuse halo. There is subtle elongation, with the galaxy appearing neither perfectly spherical nor a highly flattened disk. Evidence of recent or ongoing major mergers or tidal disturbances appears absent. The color profile is reddish, suggesting an older stellar population with a comparative paucity of active star formation. Subtle, minor disturbances or faint disk-like features cannot be ruled out due to the image's resolution and distance to the object.
