This galaxy appears to be a spiral galaxy, viewed at an angle that is neither face-on nor edge-on, presenting an intermediate inclination to our line of sight. The central bulge is prominent and exhibits a relatively smooth, concentrated light profile.

Two distinct spiral arms emerge from the central region and extend outwards. There are no clear distinct clumps of star formation within the arms. The overall arm structure appears relatively well-defined but not tightly wound. The galaxy does not exhibit obvious signs of a strong bar structure, but it's possible a weak bar structure could exist, but not seen clearly at its orientation.

There's no evidence of a major ongoing merger or significant tidal disturbances. The overall morphology suggests a relatively undisturbed spiral galaxy. The dust lanes may be present in the spiral arms, based on the change in color.
