This galaxy presents as a disk galaxy, viewed nearly edge-on. A prominent dust lane bisects the galaxy's mid-plane, obscuring the light from the central bulge. The bulge appears somewhat elongated and exhibits a subtle, rounded shape. It displays a yellowish-orange hue, indicative of an older stellar population.

The disk itself appears relatively smooth and lacks well-defined spiral arm structures, suggesting a later-type disk galaxy. The disk color transitions gradually from a pale yellow near the bulge to a fainter, bluer tinge at the outer edges. The blue color may indicate the presence of some younger stars, although star formation is not a dominant characteristic of the galaxy. Overall, the galaxy shows no signs of significant recent interactions or major mergers, though minor disturbances cannot be ruled out.
