The galaxy presents as a flattened, disk-shaped structure observed nearly edge-on. Its central region exhibits a bright, concentrated luminosity that fades towards the outer edges. The color profile appears predominantly blueish, suggesting the presence of a relatively young stellar population. The galaxy's disk shows hints of possible substructure. It's possible this is due to a weak spiral arm. There doesn't appear to be major interactions going on, however, there could be a chance of a minor disturbance.
