The galaxy presents as a luminous, elliptical form. The core exhibits a concentrated, yellowish-white glow, suggesting a high density of older stellar populations. The surrounding galactic halo displays a more diffuse, reddish-orange hue, indicative of a mix of evolved stars and potentially some dust. The overall morphology appears relatively smooth, with no prominent spiral arms or significant irregular features visible. There is a slight elongation to the galaxy's shape. No obvious signs of ongoing major mergers or tidal disturbances are apparent, although subtle irregularities cannot be ruled out at this resolution.
