The galaxy presents as an elongated, somewhat disturbed system. There is a slight indication of bluer colors, more visible in the central region. Overall, it appears relatively smooth, though there is evidence of irregular features suggesting possible ongoing or recent interactions. The galaxy exhibits a non-negligible, but not dominating light profile. This may be an indicator of a system undergoing a slow merger. It is elongated, but not necessarily disk like, but instead has a slightly more rounded, but stretched appearance. It seems to have some disturbances, which supports it undergoing a merger. 
