The galaxy presents as a centrally concentrated object with a smooth overall appearance, and an apparently elliptical morphology. The light profile suggests a significant bulge component. It has a dominant yellowish-white hue in the center which may indicate an older stellar population. Faint bluer light extends outwards to one side, suggesting a possible disk-like structure or tidal feature. There is no clear indication of spiral arms, active star formation regions, or dust lanes visible in this image. It does not appear to be undergoing a major merger, though there may be some evidence of minor gravitational disturbance.
