The galaxy exhibits a flattened, disk-like morphology. It appears elongated, with an axial ratio indicating a significant inclination relative to our line of sight. A prominent bulge is not clearly visible; the light distribution seems relatively uniform across the galaxy's body. Color gradients are present, suggesting variations in stellar populations or dust content. The central region appears to be a yellow to white color, possibly indicating an older stellar population. Toward the edges, the disk shows a bluer hue, suggesting the presence of younger, hotter stars and ongoing star formation. No distinct spiral arm structures are readily apparent in this image, giving it a somewhat smooth appearance. The size seems moderate; it is not exceptionally large or compact.