The galaxy presents a generally smooth, elliptical morphology with a bright, concentrated central bulge that appears approximately round in shape. The light distribution fades gradually from the center outwards, suggesting a lack of prominent spiral arms or distinct features usually associated with disk galaxies. The overall color profile indicates a relatively evolved stellar population, with a subtle reddish hue at the core transitioning to a slightly bluer tint in the outer regions. This may suggest a combination of older stars in the central region and ongoing, though relatively subdued, star formation in the outskirts. There is a possible faint indication of minor asymmetry or tidal disturbance in the outer halo, but overall, the galaxy appears relatively undisturbed.
