The galaxy appears as a moderately inclined disk, elongated along its major axis. The central region is bright and smooth, suggesting a prominent bulge, possibly an elliptical morphology. The bulge exhibits a yellowish hue, indicating an older stellar population. Moving outward from the bulge, the disk appears somewhat fainter and bluer, hinting at ongoing star formation. The spiral arms are not clearly defined, but there are subtle hints of features within the disk, suggesting either flocculent or tightly wound spiral structures. The overall appearance is relatively undisturbed, with no obvious signs of major mergers or tidal interactions. Based on the general smoothness, it could be an Sa or Sb galaxy.