The galaxy presents as an elliptical or lenticular system, with a dominant smooth and centrally concentrated light distribution. A subtle disk-like structure may be present but is not immediately obvious. The central bulge region exhibits a bright, luminous core, potentially indicating an active galactic nucleus.

Evidence suggests that the galaxy is undergoing or has undergone a merging event. The morphology is significantly disturbed. The primary galaxy appears to be undergoing a major merger, with significant tidal distortions visible around the main body. There is a notable plume or bridge of material extending from the main galaxy, potentially indicating the tidal interaction with the likely companion galaxy. The color gradients suggest a complex stellar population, potentially with variations in age and metallicity across different regions of the galaxy. Star formation appears subdued overall, with minimal presence of bright blue regions usually associated with massive, young stars. The overall color is relatively red, suggesting an older stellar population.
