This galaxy exhibits a disturbed morphology, potentially indicative of a recent or ongoing interaction. A faint tidal tail is visible emanating from the main galactic body, suggesting gravitational interaction with another, unseen, object.

The galaxy's color profile indicates the presence of both older stellar populations, visible in the central region, and bluer, possibly younger stars, particularly apparent in the outer regions and tidal features. The presence of blue light suggests active star formation. The central core appears compact.

There is an indication of minor irregularities or distortions in the overall structure. It may have features from a potential merging event such as a tidal tail.
