The galaxy presents as a relatively smooth, elliptical structure. It exhibits a dominant central bulge, appearing as a bright, concentrated region. The galaxy displays a somewhat elongated shape, exhibiting a cigar-like morphology rather than a perfect sphere. There is some evidence of a disk-like structure, though not sharply defined, surrounding the bulge. The outer regions show a gradual decrease in luminosity, indicating a decreasing density of stars with increasing radial distance. There is no clear indication of spiral arms or significant dust lanes. Based on its overall appearance, the galaxy is likely an evolved system with relatively low current star formation activity. We see some indications of possible past minor disturbances or interactions, but the overall structure appears relatively settled.
