The object appears to be an interacting galaxy system. A larger, primary galaxy exhibits a flattened, disk-like morphology. The central region displays high surface brightness, appearing almost stellar in nature, possibly indicating the presence of an active galactic nucleus or a dense stellar population. The light distribution of the larger galaxy appears somewhat disturbed or irregular, especially along its edges, which may indicate tidal interactions.

A smaller, companion galaxy is situated nearby. It is less elongated. The companion also exhibits a bright core. There is a clear bridge of material or tidal feature connecting the two galaxies. Both galaxies show a relatively blue color, potentially indicative of ongoing star formation activity. Overall, the system exhibits features characteristic of galaxy mergers or close encounters, where gravitational interactions are distorting the morphology of each galaxy.
