The galaxy presents as an elliptical morphology, exhibiting a smooth and generally featureless appearance. The central region displays a concentrated brightness, suggesting a substantial stellar population. The galaxy's color gradient transitions from a yellowish core to a slightly bluer outer halo, perhaps indicating varying stellar ages and compositions. No strong evidence of spiral arms or ongoing major mergers is apparent. Faint asymmetries and minor disturbances may exist on the periphery of the galaxy, but they are not prominently visible, not hinting at recent minor interactions. It appears to be a relatively isolated system with a considerable mass.
