The galaxy presents a largely smooth and elliptical morphology. It exhibits a high degree of central concentration, with a bright, prominent core. The light distribution appears to be fairly uniform and symmetrical around the center, suggesting a well-mixed stellar population. A slight ellipticity is observed, with the galaxy appearing somewhat flattened along one axis. The color profile appears consistent across the galaxy, with a subtle redder hue in the core gradually fading to a slightly bluer tinge in the outer regions. There is no discernible spiral structure or evidence of significant dust lanes. The overall appearance indicates a galaxy with a relatively old stellar population and a lack of ongoing, major star formation activity. There is no visual indication of any tidal disturbances or interactions with other galaxies.