The galaxy presents as a single, relatively smooth object with a centrally concentrated luminosity profile. The dominant color is yellow-white, suggestive of a population of older stars with lower ongoing star formation. There is a slight color gradient, with the central region appearing more yellow, and the outer regions exhibiting hints of green and some localized areas of red. The smoothness in its morphology suggests that the galaxy could be an elliptical galaxy or a spiral galaxy viewed face-on without prominent spiral arms. Faint, red-colored spots may indicate regions of ionized gas or ongoing, albeit minimal, star formation. There is no obvious disturbance, which is consistent with the majority of viewers believing the galaxy is not merging. The apparent roundness also points towards a more spheroidal structure.
