The galaxy presents a morphology that appears to be primarily smooth, with a notable deviation from a perfect elliptical shape. It exhibits a slight elongation, suggesting a possible transition towards a more lenticular form, but its most striking feature is what seems to be a tidal tail extending from the primary galactic body. This tail is diffuse and weakly luminous, indicating a potential past interaction or merger event. The central region of the galaxy displays a concentrated luminosity, potentially indicative of an older stellar population, but its overall color suggests the presence of a broader range of stellar ages throughout the galaxy. The overall appearance suggests a system that is either currently undergoing or has recently undergone some form of gravitational disturbance. The absence of clear spiral arm structures reinforces the classification as being more closely aligned with elliptical or lenticular galaxy types.
