The galaxy appears as a single, relatively smooth object with little discernible internal structure. It exhibits a generally elliptical morphology, leaning slightly towards a circular shape. There are no prominent spiral arms or a well-defined disk. It appears as a concentrated object, with a relatively diffuse halo. Color gradients across the galaxy are subtle but suggest a slightly bluer hue at the core, shifting towards redder tones in the outer regions. This could indicate a slightly younger stellar population concentrated in the galactic center. No significant tidal features or signs of recent major mergers are apparent. A very subtle disturbance can possibly be seen as slight asymmetry. The galaxy's overall color suggests a moderately evolved stellar population. There are no indications of strong, ongoing star formation.
