This galaxy presents a somewhat irregular morphology. It exhibits a dominant, centrally concentrated bulge with a yellowish hue, suggesting an older stellar population. Extending from the central bulge are fainter, less defined features that appear slightly bluer in color, hinting at regions of more recent star formation. These fainter regions are not symmetrically distributed around the bulge, indicating possible gravitational interactions or internal disturbances. There appears to be a faint tidal tail-like structure on the lower portion of the galaxy. Overall, the galaxy does not present a clear spiral or elliptical shape, but rather a disturbed or transitional morphology.
