The galaxy presents as a relatively smooth, elliptical morphology. The core is bright and concentrated, suggesting a high stellar density. The light distribution diminishes gradually from the core outwards, with no distinct spiral arm structures visible. There is a slight color gradient, the core appears yellowish-white, indicative of older stellar populations and minimal ongoing star formation. The outer regions exhibit a faint bluish tinge, possibly indicating the presence of younger, bluer stars, though these are not prominent. There's a very subtle flattening of the galaxy's shape, leaning towards a more rounded, rather than cigar-shaped, appearance. No major disturbances or clear signs of ongoing mergers are apparent from this image, although the galaxy's subtle asymmetries could suggest minor interactions in its past.
