The galaxy presents as a somewhat elliptical, disk-like structure with a high degree of central concentration. There is a distinct color gradient, shifting from a more yellow-orange hue in the central regions to a bluer, greenish tint towards the outer edges of the galaxy. This suggests the presence of older stellar populations in the core, with younger, hotter stars populating the disk. The galaxy appears largely undisturbed, exhibiting no signs of major mergers or tidal distortions. Its overall morphology is smooth, indicating that it is likely an evolved system. The light distribution implies a significant spheroidal component. No distinct spiral arms or prominent dust lanes are visible within the galaxy.
