This galaxy presents as a moderately inclined spiral galaxy, with a prominent central bulge. The bulge is observed to be yellowish-white in color, suggesting an older stellar population. Faint spiral arms are seen extending from the bulge, with a tightly wound structure. Evidence of ongoing star formation is indicated by the blueish hue present in certain regions of the arms. The disk appears relatively smooth overall, with no clear signs of major disturbances or mergers. Dust lanes are not clearly visible in the image, but this may be due to the moderate inclination angle and image resolution. The overall morphology is typical of a spiral galaxy, potentially of type Sb or Sc based on the prominence of the bulge and the tightness of the spiral arms.
