The galaxy presents as a diffuse, elliptical form with a noticeable central concentration of light. There appears to be evidence of an ongoing or recent merger event. Two distinct, bright nuclei are visible within the galactic body, suggesting the coalescence of two separate galaxies. There are faint, extended tidal features visible, potentially indicative of gravitational interactions. The overall color appears reddish, implying an older stellar population with a lower rate of star formation. The galaxy displays a smooth appearance with no distinct spiral arm structure.
