The observed galaxy presents as a roughly elliptical structure with a distinct central bulge. The core exhibits a relatively smooth and concentrated luminosity profile. Surrounding the central bulge, a fainter, diffuse halo is visible. There is evidence of some substructure within the halo, potentially indicative of disrupted material or tidal features. Blue-ish tones appear on the perimeter of the galaxy. The galaxy appears to be undergoing a merger, possibly in the later stages, or is a disturbed system, based on the irregularities observed within its structure. There is evidence of a disturbance, possibly due to interactions with another galaxy. Overall, the galaxy exhibits a disturbed morphology, suggestive of ongoing or recent gravitational interactions. 
