The galaxy presents a largely smooth, elliptical morphology, exhibiting a high degree of radial symmetry. A bright, concentrated central bulge is evident, surrounded by a more diffuse halo. The light distribution appears relatively uniform and lacks prominent spiral arms or significant dust lanes. The galaxy exhibits a slightly elongated shape, deviating slightly from a perfect circle. There is no indication of major mergers or tidal disturbances. Based on the color profile, the galaxy appears to have a population of older stars, suggesting a relatively low rate of ongoing star formation.
