This galaxy exhibits a disturbed morphology, potentially indicative of an ongoing or recent merger event. Two distinct luminous regions are visible. The region to the left appears bluer, suggesting a population of younger, hotter stars and possibly ongoing star formation. The region to the right displays a more reddish hue, which might indicate an older stellar population. A diffuse, faint tidal bridge or tail-like structure appears to connect the two regions, further supporting the hypothesis of a merger interaction. The overall structure deviates significantly from a regular elliptical or spiral form. Dust lanes are possibly present within the galaxy, but are difficult to resolve due to image resolution.
