The galaxy presents a predominantly smooth, elliptical morphology. It appears relatively compact, with a centrally concentrated luminosity profile that diminishes gradually towards the periphery. The color gradient exhibits a radial trend, transitioning from a yellowish core to a bluer outer halo. There is no readily apparent spiral arm structure or dust lane obscuration within the galaxy. The high degree of roundness indicates it might be close to face-on in our line of sight. Evident from the image is that this galaxy does not appear to be undergoing any major merger events or significant tidal disturbances.
