The galaxy exhibits a roughly elliptical morphology, though its structure appears disturbed. There is evidence of significant internal variation in color and luminosity. Mottled regions with higher intensities and bluish hues are observed across the face of the galaxy. Darker reddish regions are interspersed, creating an irregular and complex pattern. The overall appearance suggests either significant dust obscuration, recent star formation activity, or perhaps an ongoing merger event that has disrupted the galaxy's morphology. The surface brightness distribution is non-uniform. A faint halo may be present.
