The object appears as a moderately sized galaxy, exhibiting a somewhat amorphous morphology. The central region displays high surface brightness, suggesting a concentrated nucleus or core. Proceeding outwards, the intensity diminishes, yet the galactic structure still maintains coherence. The overall shape indicates a possible spiral or disk-like structure, although it is heavily perturbed. An asymmetry is apparent, with a slightly elongated and disrupted feature extending towards the left. This distortion suggests the presence of ongoing or past gravitational interactions with another galaxy, leading to tidal disturbances or a minor merger event.
