This galaxy presents a primarily smooth morphology, exhibiting a concentrated central bulge. There is a slight deviation from perfect circularity, leaning towards an elliptical shape. The color appears to be a relatively homogenous yellow-orange hue, suggesting an older stellar population with subdued star formation. Subtle indications of minor disturbances are visible, hinting at possible past interactions or mergers, but no prominent tidal tails or other major disruptions are apparent. Overall, the galaxy seems to be a relatively evolved system.
