The galaxy appears as a centrally concentrated, elliptical-like object with a smooth luminosity profile. The core exhibits a bright, yellowish hue which fades into a more diffuse, reddish halo. There is no apparent spiral arm structure or significant dust lane features visible in the image. The overall shape is more rounded than elongated, although not perfectly spherical. There is a very slight suggestion of tidal disturbance with some minor asymmetry in the outer regions, but no clear evidence of a major ongoing merger event. Based on these characteristics, the galaxy seems to be dominated by an older stellar population.
