The galaxy presents as a relatively faint spiral system, observed at an inclination angle approaching edge-on. A prominent central bulge is evident, exhibiting a concentrated luminosity gradient with a yellowish hue. This likely indicates an older stellar population dominating the nuclear region. Faint disk component surrounds the bulge, which is noticeably flattened and shows traces of spiral arm structures, though the resolution prevents clear discrimination of individual arms. These arms appear somewhat tightly wound, suggesting a possibly grand-design spiral structure. The disk exhibits a bluer color than the bulge, consistent with ongoing star formation in the disk regions. Overall, the galaxy presents a smooth appearance. There is no readily apparent strong bar feature.
