The galaxy exhibits a slightly elongated morphology. Its central region displays a bright, concentrated luminosity, indicating a likely bulge component. This core area appears to be yellowish-orange, suggesting an older stellar population. Moving outwards, the disk portion of the galaxy is visible, though somewhat indistinct. It shows hints of bluer regions that likely correspond to areas of active star formation. There appear to be some disturbances in the main body of the galaxy suggesting a possible interaction or merger in its past. The galaxy appears neither perfectly smooth nor a clearly defined spiral or elliptical shape.
