The galaxy appears as a roughly elliptical, somewhat diffuse object, exhibiting a smooth morphology. The light is concentrated towards the center, indicating a central bulge. There is an observed slight extension along its major axis. It displays a redder hue overall, implying an older stellar population and/or significant dust obscuration. No obvious spiral arm structures or prominent star-forming regions are discernible within the limitations of the image resolution. There may be minor gravitational disturbances visible.
