The galaxy appears to be a spiral galaxy, presenting an edge-on or highly inclined view relative to our line of sight. The central bulge is moderately prominent. Traces of spiral arms are visible, though the edge-on view obscures a clear definition of their morphology. A small, relatively faint bar structure may be present but is not strongly defined. The galaxy shows signs of loose spiral windings. No prominent distortions or tidal features are discernible, suggesting it is not currently undergoing a major merger. Evidence points towards it containing two spiral arms. The overall color suggests a population of older stars with ongoing star formation.
