The galaxy appears as a centrally concentrated object with a relatively smooth light distribution. It presents a roughly elliptical morphology, showing a moderate degree of roundness. There is little evidence of strong spiral arm structures or prominent dust lanes. Faint color variations are observed across the galaxy's surface, possibly indicating subtle differences in stellar populations or dust content within the galaxy. No obvious signs of major mergers or tidal disturbances are immediately apparent, although subtle irregularities in the outer regions cannot be ruled out based on this image alone.
