The galaxy presents a generally smooth and elliptical morphology. The light distribution is centrally concentrated with a bright, unresolved core suggestive of a bulge. There is a slight extension along one axis, indicating it is not perfectly spherical, though the aspect ratio suggests it is closer to round than a highly flattened disk galaxy. The color gradient appears subtle, with the central regions exhibiting a more yellowish-white hue, possibly indicating an older stellar population. Some diffuse, bluer patches are visible within the galaxy, which may be regions of ongoing star formation. There is some faint asymmetry in the outer regions and these observations could support either a minor merger or tidal disturbance.
