The galaxy presents as a single, somewhat amorphous, luminous object. The primary light emission appears to originate from a diffuse central region, with a concentration of intensity towards what appears to be an interacting system. There is evidence of a disturbance, with a plume of less intense luminosity extending outward, indicating possible tidal interactions or ongoing minor merger activity. The overall color of the system skews towards the red end of the spectrum, suggesting an older stellar population and a relatively low rate of star formation. Although some regions show younger stars, the older populations dominates overall. The morphology indicates a system that is relatively smooth, not exhibiting any clear spiral arm structure. A reasonable estimated physical size would be around 6 kiloparsecs. This galaxy is at a redshift of approximately 0.28. Finally, the galaxy is thought to have a mass around 10^11 solar masses.
