The galaxy presents a morphology that leans towards elliptical, although some features suggest potential disturbance or interaction. A significant portion of the galaxy's light appears concentrated in a central, relatively smooth region. This core exhibits a bright, yellowish-white color, indicative of older stellar populations. A less pronounced, somewhat diffuse area extends from the main body, displaying a reddish-orange hue which may signal ongoing or recent star formation. There also seems to be a possible tidal tail or distorted morphology indicative of a merger event in its past, or perhaps currently taking place.

There is no clear evidence of spiral arm structures. The overall shape is somewhere between round and elongated. Patches of varying color distribution are evident, indicating inhomogeneous stellar populations, with some regions appearing more blueish, suggesting hotter, younger stars. It appears as though it is a galaxy with some level of disturbance to its morphology. 
