The galaxy presents as a relatively compact object. Its overall morphology suggests a smooth, elliptical-like structure with a high degree of roundness. Some minor disturbances and asymmetry can be seen, possibly indicative of a past or ongoing minor interaction. The color profile shows a concentration of bluer hues near the center, grading into redder tones in the outer regions. This potentially implies a central concentration of younger, hotter stars with older stellar populations dominating the outskirts. Though smooth in appearance, the galaxy doesn't exhibit a perfectly uniform color distribution, suggesting some localized regions of differing stellar populations or dust content.
