The galaxy presents as a single, relatively smooth and elliptical-shaped object. Its color gradient suggests a higher concentration of older stellar populations, particularly towards the core, as indicated by the yellow hue. There is no clear indication of spiral arms or other disk-like features.

The galaxy appears largely undisturbed, without evidence of significant tidal distortions or ongoing major merger activity. There is no strong evidence of active star formation regions from the galaxy's color and smooth morphology, potentially indicating that the star formation rate is relatively low.
