The galaxy presents a largely elliptical morphology, appearing quite smooth and featureless across its extent. Its light profile is centrally concentrated, exhibiting a bright core that gradually fades outward into the surrounding halo. There is no apparent spiral arm structure or dust lane obscuration visible in the image. The galaxy appears fairly round, showing minimal signs of tidal disturbances or ongoing merger activity. Its color is predominantly yellowish, which could suggest an older stellar population, or a lower rate of star formation. Overall, the galaxy seems to be an evolved system consistent with a population of older stars and minimal recent star formation.
