The galaxy presents as a relatively smooth, centrally concentrated structure. There is a subtle radial gradient in luminosity, with a brighter core fading outward. The color appears relatively uniform across the galaxy, with a slight bluish tint, suggesting the presence of younger stellar populations, possibly ongoing star formation. The galaxy shows a mostly elliptical morphology, but shows some slight evidence of disturbances and asymmetries in its outer regions, indicating the potential influence of past interactions.
