The galaxy presents as a spiral type, observed at a significant inclination. The disk structure is clearly visible, exhibiting a somewhat flocculent spiral arm morphology, especially prominent when considering its bluer color. The galaxy possesses a moderately sized central bulge, with the remaining bulge is small compared to the disk. There may be a weak bar structure. The galaxy shows no signs of major mergers or significant tidal disturbances, suggesting relative dynamical isolation. Dust lanes are not very prominent. Overall, this galaxy appears to be a relatively undisturbed spiral galaxy with ongoing star formation occurring within its disk.
