This galaxy exhibits a disk-like structure with a prominent central bulge. The bulge appears yellowish, suggesting an older stellar population. The disk component shows some evidence of spiral arm structure, although these features are not sharply defined. The overall color gradient from the bulge outwards hints at ongoing star formation within the disk, with bluer regions intermixed with areas of dust obscuration. The galaxy's relatively high inclination presents a flattened appearance. There is no strong evidence of a bar-like structure, although a faint central bar is possible. The galaxy does not show any obvious signs of a major merger event, although minor tidal disturbances or interactions cannot be ruled out. It is moderately sized.
