The galaxy presents an overall smooth morphology with a centrally concentrated luminosity profile. It appears nearly round in shape, showing only a slight deviation from perfect circularity. The core exhibits a yellow-white hue, suggesting the presence of an older stellar population. Fainter, diffuse blue emission is observed in the outer regions. The overall color gradient indicates ongoing star formation. The galaxy does not show any obvious signs of major tidal disturbances or ongoing merger activity, though a hint of minor asymmetry cannot be ruled out.
