The galaxy presents a largely smooth, elliptical morphology. Its overall color is yellowish-orange, with a concentration of this color toward the central region, suggestive of an older stellar population. There is a subtle, but visible, disk-like structure with faint spiral arm hints. Evidence of a minor gravitational disturbance is apparent in the faint extensions emanating from the primary body. There is also evidence that a minor merger occurred within the galaxy itself, possibly triggering the slight star formation present within the body.
