The galaxy appears as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology with a high degree of roundness, showing no obvious spiral arm structures or a pronounced disk. The light distribution suggests a gradual decline in luminosity from the core outwards, with no significant signs of tidal disturbances or ongoing mergers. The overall color is somewhat blue, possibly indicating the presence of some younger stellar populations. There's no apparent active galactic nucleus or prominent dust lanes visible in this image. The galaxy appears to be fairly isolated.
