The galaxy presents as a slightly elongated, disk-like structure with a smooth, relatively featureless appearance. There is a notable central bulge, appearing brighter and more concentrated than the surrounding disk. The color distribution suggests a redder core possibly indicative of an older stellar population, transitioning to a slightly bluer, perhaps younger stellar population in the outer regions of the disk. There is no prominent spiral arm structure visible, though subtle color variations within the disk hint at underlying structure. The galaxy appears relatively undisturbed, with no obvious signs of recent major mergers or tidal interactions.
