The galaxy presents as a faint, elongated structure, likely a spiral seen edge-on. The disk is relatively thin and luminous, with noticeable dust lanes obscuring some of the light. The central bulge is not particularly prominent and appears to be a very small percentage of the galaxy. There are no other noticeable distinguishing features. There is some evidence of possible tidal disturbances or faint interactions, such as a faint tail or bridge feature extending from one side. The colour suggests ongoing moderate levels of star formation, and potentially some older stellar populations present. Overall, the galaxy appears to be a moderately evolved spiral with subtle signs of past or ongoing interactions.
