The galaxy presents as a relatively compact, centrally concentrated system. It appears largely elliptical in shape, with a smooth light distribution lacking prominent spiral arms or a distinct bar structure. The color profile suggests a population of primarily older stars, indicated by the redder hue concentrated towards the core. There might be some sign of disturbance in the disk, however it is quite negligible. Overall, this system seems to be a relatively undisturbed system, close to spheroidal in shape.
