The galaxy presents an elliptical morphology, appearing largely smooth and rounded in shape. A slight elongation is discernible. The central region exhibits a concentration of light, suggesting a prominent galactic nucleus or bulge. Coloration suggests a redder stellar population, indicative of older stars, with a possible slight hint of bluer star formation occurring on the edges of the galaxy. There is little evidence of significant disk-like structure or ongoing major mergers. Faint, irregular features are barely perceptible, possibly indicative of minor gravitational disturbance, but generally the galaxy appears undisturbed.
