The galaxy presents a largely smooth, elliptical appearance. It exhibits a central, bright core, surrounded by a more diffuse halo of light. There is a slight elongation to the galaxy's shape, deviating from a perfectly circular form. A color gradient is observed, with a bluer hue toward the central regions, possibly indicating ongoing or recent star formation. The outer regions appear redder, suggesting a population of older, redder stars. There is no apparent spiral structure or prominent dust lanes visible in this image. The galaxy appears relatively undisturbed, showing no signs of major merger activity, although there might be a minor disturbance in the galaxy. Overall, the galaxy appears to be a relatively massive system, consistent with its high luminosity.
