The galaxy presents as a luminous, elliptical structure. A bright, relatively featureless central bulge dominates the observed morphology. The light emanating from the core appears to be more yellowish. Fainter, bluer light is discernible toward the outer regions of the galaxy, possibly indicating ongoing, albeit subdued, star formation within a disk-like component. There is no definitive sign of spiral arms or a bar structure. A degree of asymmetry is present in the outer regions, but no definite tidal tails or strong morphological disturbances are readily apparent, however some minor disturbances seem possible. The overall shape tends toward a more elongated, cigar-like appearance rather than a perfectly spherical form.
