The galaxy presents as a centrally concentrated object with a generally smooth morphology. There is a dominant, bright central bulge region that emits primarily in the red and green wavelengths, producing a yellowish hue. The galaxy appears elliptical in shape. Fainter, diffuse emission extends outwards from the core, exhibiting a bluer color. There is no apparent spiral arm structure or significant dust lane obscuration. No other galactic nuclei or signs of interactions are readily apparent.
