The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge of high luminosity that appears nearly spheroidal in shape. Moving outward, the light gradually diffuses into a fainter, more elongated halo, indicating a transition from a dense stellar population in the core to a sparser distribution in the outer regions. 

There is no strong evidence of defined spiral arms or significant dust lanes. Subtle color variations suggest potential differences in stellar populations within the galaxy. The blue tinge around the central bulge may indicate ongoing star formation, potentially driven by a relatively high, but not extreme, star formation rate. The overall structure suggests this galaxy is either an elliptical or a lenticular galaxy, leaning toward the earlier types in the Hubble sequence. There are subtle features that suggest there may have been a minor disturbance, but likely no ongoing major merger event.
