The galaxy appears to be a relatively compact object with a smooth, elliptical morphology. A central bulge is present, exhibiting a bright, concentrated light profile. The overall color of the galaxy indicates a population of older stars, with a slight bluer tint in the inner regions suggesting possible recent star formation. No prominent spiral arms or dust lanes are visible. The galaxy appears undisturbed, with no signs of tidal features or ongoing mergers. It seems to be a relatively isolated system.
