This galaxy appears to be a relatively smooth, single structure with a somewhat elliptical morphology. The color profile suggests a population of older stars, as there is a lack of strong blue or ultraviolet emission indicative of recent star formation. There are no visually obvious spiral arms or a prominent disk component, which further supports this assessment. Some minor disturbances are not completely ruled out, but overall the galaxy presents as largely undisturbed with a lack of significant mergers or tidal features.
