The galaxy appears as a somewhat diffuse object, exhibiting a roughly elliptical morphology. The core region displays a higher surface brightness, fading towards the outer edges. There may be some tidal disturbance present to the structure of the object. The colors are consistent with a red-shifted galaxy, more pronounced in g-band emission. There is no strong visual evidence of spiral arm structures; however, there seems to be a slight clumpy structure in the outer regions which may be indicative of either some merger activity or star-forming regions. The galaxy is moderately bright.
