The galaxy presents as a somewhat smooth, elliptical object. Its core region appears bright, exhibiting a concentrated luminosity. Moving outward from the center, the light gradually diminishes into a more diffuse halo. There is a subtle elongation, deviating slightly from a perfectly circular form. No distinct spiral arm structures or prominent dust lanes are discernible from the image. Overall, the galaxy's structure appears relatively undisturbed, showing no obvious signs of a major merger event, though minor tidal disturbances cannot be ruled out. The color indices suggest a population of older stars, consistent with a relatively low ongoing star formation rate.
