The galaxy appears to be a disk galaxy viewed at a moderate inclination. A central bulge is discernible, exhibiting a yellowish hue, suggestive of an older stellar population. The disk component displays a bluer color, indicating the presence of younger, hotter stars and regions of active star formation. The overall structure seems relatively smooth, with a slight elongation of the galaxy's shape. Subtle irregularities in the disk's structure hint at possible minor gravitational interactions, but no major mergers or disturbances are apparent.
