The galaxy presents as a roughly elliptical structure with a smooth light distribution. A bright central bulge is evident, exhibiting a yellow-white hue, indicative of an older stellar population. The outer regions of the galaxy appear fainter, transitioning to a more diffuse halo. A slight asymmetry is observed in the light distribution, potentially hinting at past minor interactions. The overall morphology suggests a relatively evolved system with a dominant spheroidal component and little to no ongoing significant star formation within the last several billion years.
