The galaxy exhibits a notable disk-like structure viewed nearly edge-on. There is a visible central bulge that is slightly elongated along the plane of the disk. The light distribution appears uneven across the disk, possibly indicating the presence of spiral arm structures, although they are not clearly defined due to the edge-on perspective. The galaxy's overall color suggests a population of older stars, with a yellow-red hue dominating the observed light. There is an indication of tidal disturbance or merging event with the presence of a smaller secondary structure offset from the main galaxy body. There is a possibility of active galactic nuclei.
