The galaxy presents a morphology that appears to be undergoing significant gravitational interaction, possibly a merger. There is a luminous central region, appearing relatively smooth and concentrated, with a yellow/white hue. Emanating from this core are faint, diffuse extensions that show a bluish tint, particularly on one side. These extensions are not uniform; they exhibit irregularities suggesting tidal features or disrupted galactic arms. The overall shape is neither purely elliptical nor spiral, but rather an irregular form characteristic of galaxies experiencing gravitational disturbances. The colour gradient from the core to the outer regions suggests differing stellar populations, with potentially older stars concentrated centrally and younger, bluer stars populating the disturbed extensions. There is evidence of dust lanes or obscuring material along the outer edges of the main body, contributing to the irregular appearance. The galaxy shows hints of disturbed structure, with faint tidal tails or arcs extending outwards, indicative of ongoing gravitational interaction.
