The galaxy appears as a lenticular or edge-on spiral galaxy, elongated in shape. There is a central bulge that appears relatively smooth and homogenous in color, displaying a yellow-orange hue, suggesting a population of older stars. A faint disk extends outward from the bulge, but details are not clearly discernible; there is no evidence of spiral arm structure in this image. The overall color index implies a mature stellar population, which is consistent with a relatively low star formation rate. There is no visual indication of any active galactic nucleus (AGN) activity, mergers, or significant tidal disturbances. The galaxy seems relatively isolated.
