The galaxy appears to be a spiral galaxy, viewed at an almost edge-on inclination. A bulge is present in the center which shows an orange/red hue, potentially indicating an older stellar population. The disk is noticeably elongated perpendicular to the bulge. The disk displays blueish colors, which might be attributed to ongoing star formation within it. There is no significant morphological evidence of a major merger or tidal disturbances. There is a smooth appearance to the galaxy, with no distinct features or knotty substructure.
