The galaxy appears as an edge-on spiral, with a distinct central bulge that is brighter and more concentrated than the surrounding disk. The disk itself is relatively smooth with some mottled areas. The galaxy's color suggests an older stellar population. No signs of tidal tails or significant disturbances are visible. There is a slight asymmetry, but the galaxy appears to be relatively undisturbed. The disk is highly inclined, nearly perpendicular to our line of sight. There is no obvious active star formation.
