The galaxy presents a generally smooth and elliptical morphology. The light is concentrated towards the center, exhibiting a bright, prominent nucleus. The overall color appears to be on the redder end of the spectrum. There is a lack of discernible spiral arm structure or dust lanes. Its shape is very circular and regular. No obvious signs of active merging or significant tidal disturbances are observed. The light is well-resolved in the inner region, but becomes more diffuse towards the outer edges. Overall, the appearance suggests a galaxy dominated by an older stellar population, indicative of low star formation.
