The galaxy appears as a relatively smooth, elliptical-like structure. The central region exhibits a bright, concentrated core, suggesting a substantial stellar population. Proceeding outward, the light gradually diminishes towards the edges, indicating a decrease in stellar density. The galaxy is not perfectly spherical; there is a slight elongation or ellipticity to its shape. There are subtle color variations within the galaxy, where the central regions appear more yellowish, possibly indicating an older stellar population, and the outer regions possess hints of blue, potentially suggesting the presence of younger, hotter stars. No distinct spiral arms or prominent dust lanes are readily observable in this image. The overall morphology suggests a galaxy that has undergone significant evolution, potentially with a relatively low ongoing star formation rate. There are no indications of a major ongoing merger event, but minor irregularities may imply past interactions.