The galaxy presents as a relatively large, edge-on spiral system. A prominent bulge is visible, appearing somewhat elongated but predominantly rounded, suggesting a possible classical bulge morphology. There is no significant boxiness. The disk appears quite thin and elongated. The color profile shows a central region with a yellow-red hue. There are hints of blue tinges, perhaps related to star formation. The smooth appearance, and lack of pronounced tidal features, suggest that the galaxy is not undergoing a major merger. There are no signs of major disturbances to the overall morphology. There are no visible features of a galactic bar.
