The galaxy presents a predominantly smooth morphology. The light distribution appears highly concentrated towards the center, suggesting a prominent bulge. The overall shape is elliptical, with a high degree of roundness. There's no discernible disk component or spiral arm structure visible in the image. The color indices indicate a redder population, consistent with older stars, with a central yellow-white hue. There is no evidence of significant ongoing star formation within the galaxy, nor any major tidal disturbances or merger activity.
