The galaxy presents as a somewhat elliptical, moderately concentrated object with a smooth appearance, suggesting a relatively evolved system. It exhibits a prominent central bulge that transitions smoothly into a fainter, more diffuse halo. The color profile appears to be bluer towards the outer regions and redder closer to the center, indicating potentially younger stellar populations in the galactic outskirts and older populations concentrated within the bulge. There's a hint of minor disturbance or asymmetry in the overall structure, possibly indicative of a past minor merger or interaction, though a clear tidal tail or shell structure isn't apparent. Overall, the galaxy does not seem to present spiral arms or a pronounced disk component.
