This galaxy presents a complex morphology, likely resulting from an ongoing interaction or merger. The central region exhibits a relatively smooth appearance with a high concentration of blue light, suggesting the presence of a significant population of young, hot stars or an active galactic nucleus. This central component appears roughly rounded.

To the west, a less defined and more diffuse structure is observed. This region shows a mix of colors, with redder hues indicating older stellar populations or dust obscuration. A hint of a tidal tail or bridge-like feature can be discerned connecting this western component to the central body, suggesting a gravitational interaction.

Based on the irregular shape and apparent disturbances, it appears that the galaxy has experienced or is currently undergoing a merger or significant tidal interaction. Some level of disturbance is present in the shape of the galaxy. There is no strong definitive evidence to suggest a ongoing merger.
