The galaxy exhibits a complex morphology suggestive of an ongoing or recent merger event. The overall structure presents a somewhat amorphous shape, lacking a well-defined spiral or elliptical form. A significant portion of the galaxy's light is concentrated in a central, diffuse region, however there are multiple concentrations of light and gas. The galaxy displays variations in color, indicative of differing stellar populations or regions of intense star formation. A distinct elongated region of reddish hues extends from the central region, possibly representing a tidal tail or a stream of disrupted material resulting from gravitational interactions. Other regions of the galaxy present a greenish hue, suggesting the presence of ionized gas or younger stellar populations. The overall luminosity appears to be moderate, with some bright areas suggesting the possibility of active galactic nuclei or intense bursts of star formation, however this is difficult to determine based on morphology alone. Overall, the galaxy's disturbed morphology points to a dynamic environment shaped by interactions with another galaxy.
