The galaxy exhibits a predominantly smooth morphology, with a slight indication of disk-like structure. The galaxy is slightly elongated, displaying a relatively face-on orientation with a hint of inclination. It presents a bright central bulge with a diffuse halo. There is evidence of possible tidal disturbance or a recent minor merger event with faint wisps of material extending from the main body, specifically on one side. The color profile suggests a relatively high blue light to red light ratio in the disk and the outer regions of the galaxy, indicating recent star formation activity, with a yellow to red core with potentially older stars. There is a faint hint of a spiral arm-like structure within the disk. The disk displays several dust lanes.
