The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology leans towards elliptical, exhibiting a generally round shape with a slight elongation visible. Color gradients are noticeable, shifting from a more reddish hue in the core region to a greenish-blue tint in the outer regions. The core appears to have a high surface brightness, gradually decreasing outwards. No obvious spiral arm structures or prominent dust lanes are detected. There is no evidence of a major ongoing merger, though slight asymmetries hint at possible minor disturbances or past interactions.
