The galaxy presents as a spiral structure with a prominent, moderately sized bulge, characterized by a concentrated, bright yellowish light, suggesting an older stellar population within the core. The spiral arms are well-defined. The spiral arms exhibit a winding pattern of moderate tightness. There appear to be two dominant spiral arms extending from the central bulge, though some disruption may be present, possibly indicating an ongoing minor interaction or disturbance, but nothing drastic. There doesn't appear to be a clear edge-on disk.
