The galaxy exhibits a morphology that appears largely smooth, displaying a central bulge with a concentrated light profile. There is subtle evidence of a disk component or some other feature that breaks from perfect ellipticity, though this feature is not prominently expressed. The galaxy shows a gradual decline in surface brightness moving from the core outward.

The color profile indicates a dominance of older stellar populations, with a reddish-yellow hue in the central regions, transitioning to slightly bluer hues in the outskirts. This color variation suggests a possible difference in stellar ages or metallicities between the galaxy's core and outer regions.

There are no obvious signs of major mergers or significant tidal disturbances. The overall structure, however, suggests a possibility of minor disturbances or interactions based on subtle asymmetry in the galaxy's halo. The shape appears to be elongated, though without a distinct spiral structure.
