The galaxy presents as a moderately inclined spiral, viewed nearly edge-on. It exhibits a central bulge region which appears relatively smooth and concentrated. The disk is elongated and shows some evidence of spiral arm structure, though the resolution is not high enough to fully resolve individual arms. There appears to be a small companion, or perhaps an area of intense star formation, on one side. The color gradient suggests ongoing star formation activity, particularly within the disk component. Based on the apparent morphology, the galaxy seems to be neither a pure elliptical nor a highly disturbed merging system.
