The galaxy presents as a primarily smooth, elliptical structure with a high degree of central concentration. The core exhibits a bright, nearly uniform yellowish-white color, indicating a population of older stars. There is a very faint extension of the galaxy beyond this bright core. The color gradient suggests the presence of a slightly bluer stellar population surrounding the yellow center, which is indicative of a very low level of recent star formation activity. Overall, the galaxy appears relatively undisturbed, with no strong evidence of tidal features or ongoing major mergers. There are subtle hints of minor disturbances in its overall morphology, but further high-resolution data would be required to confirm their nature. The galaxy is round in shape and has no spiral arms. 
