The galaxy appears to be elliptical in morphology, exhibiting a smooth, diffuse light distribution. The central region is characterized by a high concentration of luminosity, appearing bright and somewhat yellow in color, indicating a population of older stars. Moving outward from the core, the luminosity gradually decreases. There is subtle evidence of a faint, disk-like structure surrounding the central bulge, but it is not well-defined. The outer regions of the galaxy have a bluer hue, suggesting the presence of some younger stars or ongoing star formation. No significant signs of tidal disturbances or major mergers are readily apparent. Overall, the galaxy appears to be a relatively undisturbed elliptical galaxy with some evidence of a possible disk.
