The galaxy presents as an approximately elliptical or spheroidal structure. The light distribution appears relatively smooth, showing a centrally concentrated luminosity profile with a gradual decrease in brightness towards the outer regions. There is no apparent spiral arm structure or a pronounced disk component visible in this image. The galaxy's color appears slightly bluer in its central region. There is a hint of minor asymmetry or possible tidal features, which is not very well resolved in this image. This is possibly indicative of past interactions or ongoing mergers. The majority of the galaxy's light seems to be contained within a region of approximately 6-7 arcseconds in diameter, appearing round in shape.
