The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears predominantly elliptical, with a diffuse, rounded shape. There is little to no evidence of spiral arm structure or a prominent disk component. The color profile suggests a population of older stars, with a subtle blueish tint toward the center and possible dust features in the lower right. No significant signs of active galactic nuclei, tidal tails, or major mergers are readily apparent, although there is a slight asymmetry suggesting the presence of a minor disturbance or possible ongoing minor merger event. The galaxy displays modest levels of ongoing star formation. The apparent size is relatively compact.
