The galaxy presents as a relatively smooth, elliptical structure. The central bulge is prominent and exhibits a high degree of luminosity, indicative of a dense stellar population. Moving outward from the center, the luminosity gradually decreases. The overall color appears to be in the yellow-red range, suggesting an older stellar population, with lower levels of ongoing star formation. The galaxy displays a generally regular, though not perfectly circular, morphology. There are no obvious signs of strong tidal interactions or major disturbances in its structure, although a very faint feature to the right of the galaxy may suggest past minor interactions or disturbance. The lack of prominent spiral arms or dust lanes further supports its classification as an elliptical galaxy.
