The galaxy presents as a relatively small, disk-shaped structure. It exhibits a discernible central bulge that appears yellowish, suggesting an older stellar population. Surrounding the bulge is a fainter, bluer disk, indicative of ongoing star formation. The disk is not uniformly bright, showing some irregular patches and possibly faint spiral arm structures, though these features are not sharply defined. Overall, the galaxy's morphology suggests an intermediate stage of evolution, with both old and young stellar populations present. There are some signs of disturbance but nothing to suggest a major ongoing merger.
