The galaxy presents as a flattened, disk-like structure, oriented approximately horizontally in the field of view. The central region exhibits a bright, concentrated luminosity with a yellowish-white hue, possibly indicative of an older stellar population or a significant dust concentration. Surrounding this core is a distinct ring-like structure exhibiting a blue color, suggesting the presence of ongoing star formation. The outer regions of the galaxy display a fainter, more diffuse halo of light, which gradually fades into the background sky. There may be some signs of minor disturbances. Overall, the galaxy appears to be an early to intermediate type spiral galaxy exhibiting features of both smooth and more structured morphologies.
