The target galaxy presents as a faint, diffuse object. Its morphology is largely smooth, lacking a distinct central bulge or spiral arm structure in the visible wavelengths. There is some slight elongation discernible, possibly indicating a disk-like structure viewed at an oblique angle, although the low resolution makes this difficult to confirm. There may be a minor disturbance in the galaxy’s form, indicating a potential interaction with another celestial object, or that it is a product of a past merger. Overall, the galaxy is observed to have a relatively even distribution of light with the exception of the slight disturbances mentioned. The color appears to be intermediate between red and blue, indicating a mix of stellar populations.
