The galaxy presents a largely smooth and featureless morphology, with a centrally concentrated luminosity profile. It exhibits a generally elliptical shape. The core of the galaxy appears yellowish-white, possibly indicating an older stellar population. Surrounding the core is a bluer halo, which could suggest a younger stellar population. There are no obvious spiral arms or strong dust lanes visible, though the outer edges show some faint, diffuse structure. There may be minor irregularities in the halo, suggesting possible past interactions or mergers. The overall color suggests a galaxy that is actively forming stars, but is also home to an older stellar population.
