The galaxy presents as a relatively smooth, elliptical-like structure, although some evidence of a disk is suggested by the slightly elongated morphology. The central bulge is prominent and appears to be the brightest region, indicating a high concentration of stars.  The light gradually diminishes from the center outward, with the outer regions appearing fainter and bluer in color. It appears as though this galaxy is not undergoing any major merging events or significant disturbances.
