The galaxy appears as a centrally concentrated, relatively smooth object. It exhibits a generally elliptical morphology, with a high degree of circularity. There are no readily apparent spiral arm structures or significant dust lane features visible in this image. The galaxy's color profile suggests a dominant population of older stars, based on the redder hues and the apparent lack of significant blue star-forming regions. There is no obvious presence of a merger event or strong tidal disruption, though minor asymmetries cannot be entirely ruled out with this image resolution. The object presents a high degree of central concentration with a smooth, fading transition into the background, which suggests a lack of active star formation.
