The galaxy appears as a single, relatively smooth, elliptical-like object. The central region exhibits a bright, concentrated luminosity. The galaxy's color distribution transitions from a yellowish-white core to a reddish outer halo, suggesting a population gradient in stellar composition and age. There is no discernible disk structure or spiral arm morphology. The smooth, featureless appearance indicates a potentially evolved system with a dominant older stellar population. Subtle irregularities may indicate minor disturbances or past mergers, but no major interactions are immediately apparent in the morphology. The galaxy seems to be fairly compact for its luminosity.
