The galaxy exhibits an amorphous morphology. There is a dominant, bright central region showing a distinct reddish hue suggesting an older stellar population, potentially a galactic bulge. Diffuse, bluer light extends outwards from this core, indicating the presence of younger, hotter stars and potentially ongoing star formation in what might be considered a disk-like structure. This region appears somewhat disturbed or asymmetrical, possibly due to minor gravitational interactions or internal dynamics. There seems to be a minor component above the main galaxy, that could be merging with the main structure. It appears brighter and yellow, and slightly elongated. The overall structure indicates that the galaxy is likely undergoing, or has recently undergone, a merger or accretion event. 
