This galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. Its overall color profile suggests a population of older stars, exhibiting a yellowish-orange hue that is indicative of lower levels of current star formation. No distinct spiral arms or dust lanes are discernible within this image. The galaxy's shape appears largely spheroidal, with a high degree of central concentration. There are no evident signs of tidal disturbances or ongoing mergers affecting the galaxy’s overall morphology.
