The galaxy presents a generally smooth and rounded morphology. The central region exhibits a concentration of light, suggesting a bulge component. There are no prominent spiral arms or a distinct disk structure visible. The color profile indicates a moderate presence of older stellar populations, particularly in the central region. The galaxy shows some minor evidence of disturbance in its overall shape, potentially hinting at past interactions or mergers. However, it doesn't exhibit any strong signs of an ongoing major merger event. Overall, this galaxy appears to be an elliptical galaxy with a relatively high mass. Based on its morphology and color, it is likely undergoing moderate levels of star formation.
