The galaxy presents as a spiral type, viewed at an intermediate angle. It exhibits a prominent bar structure that spans a significant portion of the galactic disk. Spiral arms are visible, though somewhat tightly wound and not exceptionally distinct. The bulge appears to be of moderate size relative to the disk. The overall color profile suggests a mix of stellar populations, with a yellowish hue in the central regions indicating older stars, and bluer tones visible within the disk, possibly indicating more recent star formation, although at a relatively low rate. The disk demonstrates slight irregularities, possibly indicating minor gravitational interactions or disturbances but no signs of being in a major merger. There is a faint, diffuse halo surrounding the galaxy.