The galaxy presents an overall smooth morphology. It exhibits a concentrated central bulge, appearing yellowish-orange in color. The outer regions of the galaxy show a gradual decrease in brightness and a bluer hue, suggesting the presence of younger stellar populations or ongoing star formation, albeit at a relatively low rate. The shape appears to be more elliptical than disk-like, trending towards a more rounded form with only a minor elongation evident. There is no visible evidence of any major disturbances or ongoing mergers. Based on its apparent color and structure, this galaxy is likely an intermediate-mass system dominated by older stars, with a moderate amount of ongoing star formation in its outer regions.
