The galaxy presents as a relatively smooth, elliptical morphology. It appears oblong in shape, displaying a moderate ellipticity. The color profile indicates a population of older stars, with a dominant yellowish-orange hue. There is no evidence of strong spiral arms or prominent dust lanes. Slight asymmetry is noted, potentially indicative of a minor gravitational interaction or recent merger event, though the overall structure is largely undisturbed. Star formation appears minimal based on color alone. The galaxy exhibits a concentrated central bulge, which decreases in luminosity further out.
