The galaxy presents as a generally elliptical, relatively smooth structure, lacking prominent spiral arms or a well-defined disk. Its overall shape is close to circular. There is a concentration of light in the center, suggesting the presence of a galactic bulge. Color gradients are visible, with the central region exhibiting a yellowish to pink hue, potentially indicating an older stellar population. The outer regions appear slightly bluer, which *could* suggest more recent, although subdued, star formation. There is no significant evidence of active merging events or major tidal disturbances. The galaxy shows relatively low levels of star formation.
