The galaxy exhibits a somewhat amorphous morphology, lacking a clear spiral structure or elliptical shape. It is characterized by a bright, concentrated central region that appears almost stellar in nature, suggesting a potentially active galactic nucleus or a region of intense star formation. The central region is surrounded by a more diffuse halo of light. Some irregularities are observed in the outer regions, with hints of possible tidal features or distortions, which might indicate past or ongoing interactions with another galaxy. Overall, the galaxy appears to be undergoing some form of disturbance to its structure. The galaxy appears relatively compact, with a noticeable brightness.
