The galaxy presents as a singular body with a central bulge and what appears to be a tidal tail indicating recent or ongoing interaction with another galaxy or object. The primary light emission is concentrated in the central region, showing a bright and concentrated core, suggesting a high density of stars and possibly an active galactic nucleus. The shape of the galaxy is not perfectly elliptical; the overall structure shows significant irregularity. 

The galaxy exhibits a color gradient. The central region appears to be more blue. Given its structure, there are indications of a dynamically active system possibly due to interactions that have triggered star formation. This is further supported by the tidal tail, a common feature in merging or interacting galaxies.
