This galaxy exhibits a complex morphology. A central, bright, yellowish-white region appears dominant, likely representing a concentrated nucleus or bulge. Extending outwards is fainter material, possibly indicative of a disk structure. The galaxy has a moderately elongated shape, neither perfectly spherical nor highly flattened. 

There is evidence of disturbances in the galaxy’s structure, particularly on one side where a plume or tidal feature emerges. This suggests possible interaction with another galaxy or a past merger event.

Color variations are present, with the central region showing a yellower hue, potentially indicating an older stellar population. The outer regions show hints of bluer colors, which could be attributed to ongoing star formation within a disk component. Overall, the galaxy seems to be undergoing some form of evolutionary process, as suggested by the features observed.
