The galaxy presents as a somewhat rounded object, though not perfectly circular. The light is primarily concentrated in the center with a relatively smooth decrease of light intensity moving outward. There appears to be a slight elongation or asymmetry to the light distribution, hinting at an oblate spheroidal shape rather than a perfect sphere. The color is somewhat uniform, with a hint of redness. There is no distinct evidence of spiral arm structures or other prominent features such as dust lanes. This suggests the galaxy is likely an elliptical galaxy or a lenticular galaxy viewed at a shallow inclination. Based on the overall appearance, there is no apparent major ongoing merger activity.
