The galaxy presents as a single, relatively smooth and centrally concentrated object. It appears elliptical in shape, with an axial ratio close to unity. The core displays a bright, diffuse glow, potentially indicative of a dense stellar population or active galactic nucleus. There is some faint blue hue in the outer regions, possibly suggesting the presence of younger, hotter stars in the periphery, however the bulk of the galaxy appears to be composed of older stars. No significant signs of spiral arms, bars, or major disturbances from ongoing mergers are clearly discernible. A very slight asymmetry is present, but overall the galaxy displays little structural complexity in this image.
