The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a round morphology. The color profile suggests a dominant population of older stars, with a central yellowish-orange hue. There's a slight indication of bluer regions in the outer edges, indicating a possible small degree of on-going star formation. The overall structure appears undisturbed, with no apparent signs of recent major mergers or tidal interactions. There appears to be no strong spiral arm structure or a prominent central bar feature.
