The galaxy appears as a single, smooth object, with a concentrated central bulge that is slightly elongated along its vertical axis. The light from the galaxy is concentrated and centrally-dominant, lacking any distinct spiral arms or a well-defined disk structure. The overall color suggests an older stellar population and little on-going star formation, though the bluer color suggests some. There is a possible interaction with a smaller, more compact companion galaxy on its lower-right side. A fraction of the light from the galaxy may be scattered across a larger area, suggesting a faint stellar halo. There's a weak indication of a minor gravitational disturbance, possibly due to the interaction with the companion galaxy.
