This galaxy appears as a moderately bright, diffuse object with a primarily yellowish-red hue. The light distribution is fairly smooth, suggesting a spheroid-dominated morphology. It shows signs of an interacting system; at least one more galaxy is apparently in the process of merging with it. There is evidence of some disruption in the main body's morphology, suggestive of tidal forces and gravitational interactions, even potentially merging with other nearby structures. The galaxy overall appears relatively evolved, indicative of older stellar populations dominating its luminosity.
