The galaxy presents as a spiral type, observed at an oblique angle relative to our line of sight, likely less than 45 degrees. A prominent central bulge exhibits a yellowish-white hue, indicative of an older stellar population. Extending from the central bulge are two prominent spiral arms. These arms are tightly wound around the central bulge, indicating that the galaxy is likely a Sa or Sb type spiral. There is also a bar in this galaxy that exhibits a strong signal. Patches of bluish light are observed within these arms, suggestive of ongoing star formation activity. There are no signs of other galaxies in the immediate vicinity so it seems to be free of tidal disturbances. The overall structure shows no pronounced distortions.