The galaxy exhibits a generally smooth morphology, with a shape somewhere between round and elongated. A prominent central bulge is apparent, showing a concentration of older stellar populations, indicated by its reddish-orange hue. Surrounding the bulge is a fainter, bluer disk, suggesting the presence of ongoing star formation. No significant spiral arm structures are readily visible, although a slightly irregular shape suggests the possibility of minor disturbances. The galaxy doesn't seem to be undergoing any major merger events.
