The galaxy presents an overall elliptical morphology, appearing elongated with a relatively smooth light distribution. The central region exhibits a brighter, more concentrated luminosity profile, suggesting a prominent galactic nucleus. Proceeding outwards, the light gradually diminishes, forming an extended halo or bulge component.

There's evidence of a subtle color gradient, with the central region appearing somewhat bluer, possibly indicating the presence of a younger stellar population. The outer regions transition towards redder hues, indicative of older, cooler stars. The pronounced ellipticity of the galaxy suggests it is viewed at a significant inclination angle relative to our line of sight. There are no obvious signs of spiral arms or other distinct features such as dust lanes or star-forming regions. The smoothness of the galaxy's structure points towards a likely lack of recent major mergers.
