The galaxy presents a spiral morphology, characterized by a central bulge with a yellow hue, indicative of an older stellar population. Spiral arms extend outwards from the bulge, though they appear somewhat diffuse and ill-defined. The arms exhibit bluer regions which possibly denote pockets of recent star formation, although these regions are not sharply resolved. The overall color of the galaxy suggests intermediate to low star formation activity, with a more dominant population of evolved stars. The galaxy appears relatively isolated and does not show signs of major interaction or merging events, but there may be some minor disturbances. It is primarily face-on, with the disk almost perpendicular to our line of sight.
