This galaxy exhibits a complex morphology. The light distribution suggests a disk-like structure but with noticeable disturbances. A significant portion of the galaxy appears amorphous, with irregular light patterns.

There is evidence of possible tidal features or disrupted arms, indicating past or ongoing interactions. The core region appears relatively bright, hinting at a possible active galactic nucleus or a dense stellar population. The galaxy displays a range of colors, from bluish hues in some regions, possibly indicating younger stellar populations and active star formation, to reddish tones in other areas, likely representing older stars or dust obscuration. The overall structure points toward a system that is either undergoing a merger or has recently experienced one, leading to the observed distortions in its shape. The presence of dust lanes is also suggested in the image.
