The galaxy presents as a largely elliptical morphology, exhibiting a smooth, concentrated light profile with a dominant central bulge. There is little evidence of a distinct disk structure or spiral arms; the object appears rather homogenous. The primary color is yellowish-orange, which is typical of galaxies with older stellar populations. A subtle green tint is evident in the outer halo, suggesting ongoing, but subdued, star formation. There are no obvious signs of any major disturbances such as tidal tails or distorted morphology which might indicate a recent or ongoing merger event. The galaxy appears isolated.
