The galaxy presents a generally elliptical morphology, although not perfectly circular. It appears to be relatively smooth in structure, with little visible evidence of spiral arms or distinct features. The light is concentrated towards the center in what would suggest to be a bulge, with a gradual decrease in luminosity towards the edges. The central region exhibits a yellowish-white hue, potentially indicating an older stellar population, while the outer regions show hints of bluer light, which could be indicative of more recent star formation or a younger population of stars. There is only the slightest hint of some tidal distortion or asymmetry, suggesting a possible, ongoing minor interaction with a satellite.
