The galaxy presents as a single, relatively smooth object with a concentrated central bulge. The overall shape is elliptical, appearing somewhat elongated or oblate rather than perfectly spherical. The luminosity profile appears brightest at the core, with a gradual decrease in brightness towards the outer regions. There is little evidence of distinct spiral arms or other significant features. The color of the galaxy appears to be overall redder, particularly towards the central region, potentially indicating an older stellar population. There may be some slight blue areas at the edges, perhaps suggesting some star formation at the edges. There are no obvious signs of tidal distortions or ongoing mergers.
