The galaxy presents a generally smooth and rounded morphology. The central region exhibits a concentrated luminosity, appearing significantly brighter and redder than the outer regions. There is a slight hint of disk-like structure and some diffuse features, but the overall light distribution is relatively uniform without prominent spiral arms or bar structures. The color gradients suggest a possible aging stellar population concentrated in the core, with bluer, potentially younger stars more sparsely distributed in the outer regions. There are faint, disturbed features surrounding the galaxy.
