The galaxy presents as a moderately luminous, disk-shaped system with a centrally concentrated bulge. The bulge exhibits a yellowish-orange hue, suggesting an older stellar population. The disk component appears somewhat inclined to our line of sight, displaying a flattened elliptical shape. Within the disk, some subtle hints of spiral arm structure are visible, though not sharply defined. There is also a suggestion of a small amount of star formation within the disk. The disk and halo present with a more blue hue, which suggests the presence of ionized gas. Overall, the galaxy appears relatively undisturbed, lacking any major signs of recent mergers or tidal interactions.
