The galaxy presents as a relatively smooth, elliptical-like structure. Its color profile indicates a dominant population of older stars, with a yellowish-red hue concentrated towards the center and gradually fading outwards. There is a central bulge which is quite prominent, with a diffuse halo surrounding it. No distinct spiral arm structures or prominent dust lanes are discernible within this image. There may be some signs of minor gravitational disturbance, but the galaxy otherwise seems to be isolated. The overall morphology suggests this is a massive galaxy with a relatively low star formation rate.
