The galaxy presents a predominantly smooth morphology, exhibiting a near-perfectly rounded shape. Its color profile suggests an evolved stellar population, with a dominant yellowish hue concentrated towards the galactic center. The light appears more diffuse as we move outward, and the presence of a disk is not obvious, which is consistent with an elliptical galaxy classification. There is no significant distortion of the galaxy's structure, suggesting there are no major ongoing merger events. The galaxy is relatively compact, without the presence of well-defined spiral arms or prominent features.
