The galaxy presents a complex morphology, potentially indicative of an ongoing or recent merger event. The primary structure appears to be elliptical, with a relatively smooth light distribution across the main body. There is a secondary component exhibiting a more disturbed morphology, appearing as a tidal tail extending outwards, suggesting gravitational interaction with another galaxy or object. The light from the galaxy exhibits a redder color, which suggests an older stellar population.

There may be active galactic nuclei activity given the relatively bright core that has an apparent magnitude between 17-20. The overall color suggests that the stellar population in this galaxy is relatively old. It should be noted that the galaxy exhibits signs of disturbance indicating it may be in the process of merging.

