The galaxy presents as a disk galaxy, observed nearly edge-on. A distinct bulge is visible, exhibiting a somewhat rounded morphology. The disk component shows a subtle gradient in color, suggesting potential variations in stellar populations or dust obscuration across its extent. The galactic disk appears relatively smooth, without any obvious large-scale spiral arm structure. There is no strong evidence of ongoing major merging activity or significant tidal disturbances affecting the morphology of the galaxy, though minor disturbances may be present. Overall, the galaxy seems to be a relatively isolated system.
