This galaxy presents as a moderately bright object with a generally smooth morphology, although some subtle features are discernable. The central region exhibits a concentrated luminosity, appearing almost spheroidal in shape. The light profile decreases gradually from the core outwards, and the overall hue is suggestive of a population of older stars dominating its stellar content.

There is evidence of minor disturbances, and the outer regions may contain some faint, diffuse extensions of light, but the image is not high resolution enough to define this accurately. The galaxy appears to be an elliptical or lenticular galaxy with a low rate of star formation, and a likely stellar mass of ~ 10^11 solar masses. 
