The galaxy presents a complex morphology suggestive of an ongoing or recent merger event. A prominent tidal tail extends from the main galactic body, displaying a curved structure. This tail exhibits a diffuse luminosity gradient, transitioning from a brighter, more concentrated region near the galaxy's core to a fainter, more dispersed outer edge.

The main body of the galaxy appears disturbed, lacking a clearly defined spiral structure. The central region shows a brighter concentration, likely indicative of a galactic nucleus. Patches of what appear to be active star formation are distributed throughout the distorted disk, contributing to its irregular appearance. There's a hint of dust lane structure, though its visibility is obscured by the overall disturbance. The colour profile suggests the presence of both older stellar populations, visible in the yellow-red hues of the bulge, and younger, hotter stars, which contribute to the bluer tints observed within the star-forming regions.
