The galaxy presents a primarily smooth and elliptical morphology, with a high degree of central concentration. The core region exhibits a yellow hue, potentially indicative of an older stellar population dominating this area. There is a slight elongation observed, moving towards a cigar-shaped structure. A faint, diffuse reddish area can be seen to the side of the galaxy core. The bulk of the galaxy appears to be undisturbed, with minimal evidence of significant merger activity. The faint blue-ish region is on the opposite side of the red region; these blue and red regions might be dust or areas of slight disturbance. Star formation may be ongoing, although not at a high rate, if we use the blue area as our basis. 
