The galaxy presents as a centrally concentrated object, exhibiting a smooth, elliptical morphology. The light profile is brightest and yellow at its core, indicating a higher concentration of older stellar populations within the bulge. Diffuse, greenish light extends outward from the core, suggesting the presence of younger stars or ionized gas in the galaxy's outskirts. The overall form lacks any clear spiral arm structure or significant morphological disturbance, pointing to a relatively undisturbed and evolved system.
