The galaxy presents as a spiral galaxy with a moderately sized bulge. The spiral arms are prominent and well-defined, exhibiting a two-arm structure with a medium winding pattern, loosely wound and extending outwards from the central bulge.

The bulge displays a yellowish-white color, suggesting an older stellar population, while the spiral arms exhibit bluer regions, indicative of younger, hotter stars and ongoing star formation. There appears to be a weak bar structure visible within the central region. The overall morphology indicates that the galaxy is relatively undisturbed, with no significant signs of major mergers.
