The galaxy presents as a slightly elongated, elliptical morphology. It exhibits a smooth, relatively featureless appearance, lacking prominent spiral arms or distinct dust lanes. The central bulge region displays a yellowish hue, indicative of an older stellar population. A diffuse halo surrounds the galaxy, with a bluer tint, suggesting the presence of younger, hotter stars in the outer regions. There is no immediate indication of a major ongoing merger, though subtle asymmetries hint at possible minor interactions in its recent history. The overall color suggests the galaxy is in a transitional stage, perhaps evolving from a more actively star-forming system to a passively evolving elliptical.
