The galaxy presents as a single, relatively smooth object with a yellowish-orange hue. Its morphology is generally elliptical, exhibiting a concentrated central bulge and a less defined outer region. There is no apparent spiral arm structure or significant dust lane obscuration visible in this image. The galaxy appears to have a fairly consistent luminosity profile from its core outwards, with a slight decrease in brightness towards the edges. No obvious signs of major ongoing mergers or tidal disturbances are detected in this image, indicating relative gravitational stability.
