The galaxy presents as a largely featureless, smooth elliptical morphology. Its overall shape approximates a rounded form, with minimal deviation towards elongated or irregular structures. The dominant coloration is a yellowish-orange hue concentrated towards the core, suggesting an older stellar population. A subtle color gradient is present, transitioning to slightly redder tones at the periphery. There is very little evidence of spiral arm structure or dust lane obscuration. The observed smoothness suggests the absence of major ongoing merger events, although a possible minor disturbance might be present on the lower left of the main body. The galaxy appears relatively isolated.
