The galaxy presents a generally smooth, elliptical morphology. Its light profile suggests a centrally concentrated bulge, which is slightly elongated. The galaxy exhibits a distinct color gradient, transitioning from a bluer core to redder outer regions. This color variation implies a radial change in stellar populations, with younger, hotter stars concentrated toward the galactic nucleus and older, cooler stars dominating the periphery. There is no discernible spiral arm structure or evidence of recent major mergers. Minor irregularities in the galaxy's outer halo might suggest past interactions or minor disturbances. The overall appearance indicates a galaxy undergoing passive evolution, where the rate of star formation has decreased in the past, but continues to persist to some extent.
