The galaxy presents as a relatively bright, well-defined object. It appears largely smooth in texture with a slightly elliptical, but close to round, morphology. There is evidence of a minor disturbance and possible interaction or merger. The disturbance is small compared to the main body of the galaxy.

The galaxy exhibits a color gradient. There is a dominant red core/center. This could be due to older stellar populations and/or dust obscuration. The outskirts are bluer, indicative of younger stars and ongoing or recent star formation. The galaxy has an estimated physical size in that is approximately 3 kpc across.
