The galaxy appears to be a relatively bright, disk-shaped system. Its central region exhibits a yellowish hue, suggesting an older stellar population. Moving outward from the center, there's a noticeable transition to a bluer color, indicating the presence of younger, hotter stars in the outer disk.

There is evidence of disk features or spiral arm structures, though these are not highly defined. The galaxy appears to be relatively isolated, with only minor signs of disturbance or interaction with other galaxies. Its overall shape leans towards being rounded.
