The galaxy exhibits a morphology indicative of a spiral type, with relatively well-defined spiral arms emanating from a central bulge. The arms appear somewhat flocculent. The color gradient suggests active star formation within the arms. There may be a faint bar-like structure bisecting the central bulge. There appears to be a galaxy that is merging with the spiral galaxy, with an interacting, distorted shape. There is evidence of strong tidal forces, possibly indicating a merger in progress. The central bulge shows moderate emission. Overall, the galaxy displays intermediate luminosity and a morphology suggesting active star formation and ongoing gravitational interactions.