The galaxy appears relatively small and compact. It exhibits a bright, concentrated central region, possibly indicative of an active galactic nucleus or a dense stellar population. The overall color is primarily bluish-white, suggesting the presence of younger, hotter stars. The morphology appears disturbed and asymmetric. Faint extensions or tidal features are present, indicating possible interactions with another galaxy or past merger events. The galaxy disk is not well-defined, and the spiral arms, if present, are difficult to discern. Overall, the galaxy shows features that support the hypothesis of a dynamic history involving gravitational interactions.
