The galaxy presents as a relatively smooth, elliptical morphology. The light is concentrated centrally, with a gradual decline in surface brightness towards the outer regions. There is minimal evidence of spiral arms or distinct features in the disk. The shape is somewhat elongated but it would not be considered as a cigar shaped galaxy. There is no strong evidence of any significant disturbances due to mergers or interactions with other galaxies. The central region of the galaxy exhibits a yellow-white hue, potentially indicative of an older stellar population, while the outer regions appear slightly bluer, which may suggest some ongoing star formation. 
