The galaxy presents a somewhat amorphous structure, appearing largely smooth with a slightly elongated form. It exhibits a central, brighter region, potentially indicating a higher density of stars or active galactic nuclei activity, surrounded by a more diffuse halo. The primary body of the galaxy has a moderate color gradient, transitioning from a slightly bluer hue in its outer regions to a subtly redder tint in its core. A faint, elongated structure extends from the main body. There is evidence of potential gravitational interaction or minor disturbances, possibly indicating a merger event. This conclusion is drawn from the disturbed structure and the hint of asymmetry in the overall form.
