The galaxy presents as a spiral galaxy, viewed at a slight angle. The disk component is prominent and exhibits a distinct spiral structure. The spiral arms appear tightly wound around a central bulge, with two arms being most dominant. The bulge is small relative to the disk, and its color appears more yellow, possibly indicating an older stellar population compared to the bluer disk. There is no apparent bar structure bisecting the central region. The spiral arms appear blue, potentially indicative of ongoing star formation within these regions. The galaxy shows no signs of major mergers or significant tidal disturbances, although some minor asymmetry in the arm structure might suggest past interactions or internal processes. Overall, the galaxy seems to be a relatively well-defined spiral with a moderate amount of star formation occurring within its arms.
