The galaxy appears as a single, relatively smooth object. It exhibits a centrally concentrated luminosity profile. The core region presents a bright, yellow-white hue, potentially indicative of an older stellar population or dust reddening. There is a slight gradient in color, with the outer regions showing a faint bluish tinge, possibly suggesting the presence of some younger stars, but the light is mostly yellow. No prominent spiral arms, bars, or distinct morphological features are discernible. The overall shape is roughly circular or elliptical, with no obvious signs of significant tidal disturbances or ongoing major mergers. The galaxy appears generally undisturbed, with a high degree of symmetry. The light is somewhat diffuse around the edges of the galaxy, not tightly packed.
