The galaxy presents as a slightly asymmetric, disturbed spiral. A distinct central bulge exhibits a yellowish hue, indicative of an older stellar population. The spiral arms are somewhat indistinct, with a patchy distribution of bluer regions that likely represent areas of ongoing star formation. The overall shape of the galaxy seems to be irregular suggesting the possibility of minor gravitational interactions or perhaps a past merger event. A notable feature is its disk, seen at an angle that is neither completely face-on nor edge-on. There is a small hint of a disturbance but there does not appear to be a significant merger underway.
