The galaxy exhibits an irregular morphology, deviating from a clear elliptical or spiral structure. There is evidence of significant disturbance in the overall form. The galaxy's light profile appears relatively diffuse, suggesting either a smooth distribution of stars or a more chaotic distribution due to ongoing interactions. There seems to be a region of enhanced blue light, possibly indicating ongoing star formation within that area. A fainter redder tail or distortion on one side suggests the possibility of a minor or major merger event. This area of enhanced brightness on one side may also result from tidal interactions with another galaxy, or simply be an area of localized star formation that makes the rest of the galaxy appear bluer overall. There's also a smaller portion that seems slightly detached from the main body, supporting the merger or tidal interaction hypothesis. 
