The galaxy presents as a relatively small, distant object. Morphologically, it exhibits characteristics suggestive of a transitioning system. The primary body appears smooth and elliptical.

There are visible irregularities in its structure, suggestive of tidal distortions or interactions. A faint, extended structure appears to emerge on one side of the galaxy, possibly a tidal tail or plume resulting from a past interaction. Color gradients across the galaxy are subtle but discernible. The central region exhibits a yellowish hue, suggesting an older stellar population. The outer regions appear slightly bluer, hinting at regions of ongoing star formation. The overall structure is somewhat disturbed, indicating a possible merger event. This is further supported by the disrupted morphology and faint tidal features. Overall, this galaxy appears to be a massive, evolved system undergoing some form of interaction or disturbance, leading to the observed morphological complexities and possible changes in its star formation activity.
