The galaxy presents as a relatively smooth, luminous object. Its overall shape is elliptical, exhibiting a high degree of roundness. No distinct spiral arm structures or a prominent disk component are discernible. The galaxy appears to be a single, cohesive entity, with no immediately obvious signs of major mergers or significant tidal disturbances. There is a suggestion of a slight color gradient, with the core region possibly exhibiting a yellower hue compared to the outer regions of the galaxy, which might indicate differing stellar populations. The galaxy has a fairly uniform appearance.
