The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, with an apparent lack of distinct spiral arm structures. The light distribution suggests a high degree of central symmetry with gradual fading towards the outer regions. Color gradients within the galaxy are subtle. The central region appears somewhat redder, potentially indicating a population of older stars, while the outer regions show a slightly bluer hue, possibly reflecting ongoing star formation, although at a relatively low rate. No prominent dust lanes or active galactic nuclei are obviously visible in the image. There might be some minor disturbances hinting at a prior interaction or merger event, but the overall structure is largely undisturbed.
