The galaxy presents a predominantly smooth visual texture. A bright, concentrated central bulge dominates the structure, exhibiting a near-spherical morphology. The surrounding disk, while present, appears somewhat subdued and displays a comparatively fainter luminosity. There is a slight elongation in its overall shape, suggesting a moderate deviation from a perfectly circular form. Faint hints of asymmetry are detectable, potentially indicative of past minor interactions or internal disturbances. The galaxy’s color profile suggests a relatively evolved stellar population, trending towards redder hues. There are no apparent signs of active star formation regions. The overall structure implies a system that has largely completed its morphological transformation.
