The galaxy appears to be a spiral galaxy at an approximate redshift of 0.106, as indicated by spectroscopic measurements. It is observed at an inclination that prevents precise determination of the exact number of spiral arms, but a flocculent morphology is likely due to the fuzzy and undefined arms. There are two or three primary arms. The winding of the spiral arms can be described as medium to tight. The presence of dust lanes are subtly visible. The central bulge is clearly visible and appears of moderate size compared to the disk. While the central region exhibits a yellowish hue, suggestive of an older stellar population, the disk displays a bluer color, likely indicative of ongoing star formation. There is no apparent strong bar structure bisecting the central region. A weak bar structure is also unlikely. There is no evident sign of a major ongoing merger. The galaxy shows a mostly undisturbed structure, although minor disturbances cannot be ruled out. The apparent size indicates that it is smaller than our own Milky Way galaxy.