The galaxy presents an elongated, disturbed morphology. The central region exhibits a primarily smooth appearance, transitioning outwards to less defined structures. Evidence suggests a possible ongoing or recent interaction with another galactic body, indicated by tidal features, or possibly a merger event. The system is slightly brighter at one end, suggesting a more dense concentration of stars or active galactic nucleus, with a bluer hue. Color variation within the galaxy indicates varying stellar populations or dust obscuration. Some areas exhibit a redder color, which would point to older stars or dust. The galaxy displays a generally featureless disk, with potential disturbances from a merger event. A possible companion object or tidal tail extends from the main body. Further analysis is needed to confirm the nature of the observed disturbances and to determine the precise mechanisms shaping the galaxy's morphology.
