The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and concentrated light profile. It appears largely featureless. The light is most concentrated in a central bulge that transitions smoothly into a fainter, more diffuse halo. The galaxy's overall shape appears somewhat elongated, deviating slightly from perfect circularity. The color indices indicate a population of older stars, with the light trending towards redder wavelengths. There is no evidence of spiral arms or significant dust lanes. Based on its overall appearance and color, the galaxy appears to be relatively quiescent, with a low rate of star formation. There is no evidence of any major mergers. The galaxy may be interacting with a dwarf galaxy as there are faint distortions in the outer regions.
