The galaxy presents as an edge-on spiral with a prominent, bright central bulge. The bulge exhibits a smooth, rounded morphology. The disk component is thin and elongated, with a relatively consistent width along its visible extent. There is some evidence of faint, diffuse material extending outwards from the main disk, potentially indicating a low level of recent or ongoing star formation. No significant tidal features or signs of major mergers are apparent. The galaxy appears relatively isolated.
