The galaxy presents as a relatively smooth, elliptical-like structure. There is a concentrated central bulge, which appears a slightly yellowish-white hue, suggestive of an older stellar population. Surrounding the bulge is a more diffuse, bluer halo, potentially indicative of ongoing, though perhaps relatively low, levels of star formation. The galaxy exhibits a generally rounded morphology, with only very slight deviations from a perfect circular shape. There is no visually apparent evidence of major tidal distortions or significant merger activity.
