The galaxy presents a generally smooth, elliptical morphology. The light distribution indicates a centrally concentrated bulge component with a diffuse, extended halo. The primary color is yellowish-white, suggesting a stellar population dominated by older, lower-mass stars. There's a slight elongation visible, indicating a deviation from perfect spherical symmetry, tending towards a cigar shape. A subtle hint of bluer color is detected at the periphery. No distinct spiral arms, dust lanes, or active galactic nuclei are apparent. The overall structure appears relatively undisturbed, showing no signs of major merging events, with only a slight, potential minor disturbance on the far right.
