The galaxy presents as a relatively smooth structure, generally elliptical in appearance, but with a slightly elongated morphology. The central region exhibits a brighter, more concentrated luminosity. The overall color profile suggests a mixture of stellar populations, with a tendency toward slightly bluer hues in the outer regions, possibly indicative of some ongoing star formation, albeit at a low rate. There are no immediately apparent tidal features or signs of a major ongoing merger, although a minor disturbance within the galaxy cannot be ruled out. The overall appearance points towards a galaxy that is neither a pure elliptical nor a fully developed spiral, existing somewhere between these two classifications, possibly in the form of a lenticular galaxy.
