The galaxy displays a prominent disk structure, observed at a significant inclination angle. Its morphology suggests classification as a spiral galaxy. Two distinct spiral arms are discernible, exhibiting a relatively loose winding pattern. A central bulge is present, appearing neither particularly dominant nor negligible in size. There is an indication of a bar-like structure within the central region of the galaxy. The galaxy exhibits signs of internal structure, with varying concentrations of stellar populations and possible ongoing star formation activity within the spiral arms. The overall color profile indicates a relatively young stellar population and ongoing star formation. There are no signs of a major merger, but there are possible minor disturbances within the galaxy's morphology.