The galaxy appears as a relatively smooth, elliptical-like structure. It exhibits a centrally concentrated luminosity profile, with a bright, yellowish core that gradually fades into the surrounding halo. There is no discernible spiral arm structure or prominent dust lanes visible in this image. The galaxy appears generally rounded with no obvious signs of any major disturbances or mergers. The color suggests an older stellar population, with a lower rate of on-going star formation. The light is dominated by redder wavelengths.
