The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape appears elliptical, deviating slightly from perfect circularity. The light distribution suggests a prominent bulge component, characterized by a yellowish-orange hue, indicating an older stellar population. The outer regions display a fainter, more diffuse structure with hints of a bluish tint, which may indicate younger stars and possibly some ongoing star formation. There is a lack of distinct spiral arms or other prominent features usually associated with actively star-forming galaxies. Subtle irregularities in the outer regions may indicate minor gravitational interactions or past merger events. The galaxy's radial light profile decreases smoothly from the center outwards, consistent with an early-type galaxy classification.
