The galaxy presents as a spiral, displaying a well-defined disk structure. The arms exhibit a morphology characterized primarily by two spiral arms, and they appear somewhat tightly wound around the galactic center. A prominent central bar structure traverses the galactic nucleus, contributing to its overall shape. The bulge component appears of moderate size in relation to the rest of the disk. There is evidence for ongoing star formation within the spiral arms, as suggested by the subtle presence of blue-ish regions tracing the arm structure. There are no obvious signs of major mergers or significant tidal disturbances, although subtle irregularities in the outer disk may indicate minor interactions or past merger events. The galaxy shows a color gradient, with the central bulge appearing yellower than the bluer spiral arms. The overall luminosity is high and the galaxy has a redshift of approximately 0.046.
