The galaxy presents a roughly elliptical morphology, with a dominant smooth component. There is a faint, extended halo surrounding the central region. Evidence of significant tidal features indicates that the galaxy has likely undergone a recent or ongoing merger event. The central region shows a concentration of light, potentially indicative of an active galactic nucleus or a dense stellar population. Some subtle color variations exist across the galaxy, with bluer regions appearing more distally and redder regions in the central area. This could be indicative of varying stellar populations. It is difficult to determine the exact morphological type due to the ongoing interaction, but it appears to be trending toward an elliptical form.
