The galaxy presents a generally smooth morphology, exhibiting an elliptical shape. Its color profile suggests a dominance of older stellar populations, emitting primarily in the redder wavelengths with a moderate contribution from green. The light is concentrated towards the center suggesting a high mass concentration, while the outer regions fade gradually into the background. The galaxy is relatively undisturbed, showing no obvious signs of major mergers or tidal interactions. The slight elongation suggests it may not be perfectly spherical, but rather an oblate spheroid. Star formation appears to be subdued, if present at all. Overall, the galaxy appears to be a passively evolving system.
