The galaxy appears as a somewhat elliptical structure, with a bright, concentrated central bulge. There is a noticeable absence of well-defined spiral arm features, suggesting a relatively smooth morphology. The overall color is yellowish-orange, potentially indicating a stellar population that is dominated by older stars. The galaxy exhibits a modest degree of asymmetry, hinting at a possible interaction or past merger event. The outer regions are significantly fainter than the core, with a gradual decrease in luminosity as distance from the center increases. 
