The galaxy presents as a largely smooth, elliptical-like structure with a round morphology. It exhibits a concentrated central bulge, which appears yellowish, suggesting an older stellar population. The outer regions of the galaxy are less defined, with a gradual decrease in luminosity toward the edges, with little evidence of spiral arms or distinct features. There may be very minor disturbances, but appears to be no major ongoing mergers. The galaxy shows a red shift, indicating it is moving away from us, consistent with the expansion of the universe. Star formation is likely present at a low rate.
