The galaxy presents as a slightly elongated, luminous object with a prominent central bulge. The morphology appears generally smooth, with a high degree of central concentration. There is a suggestion of a disk component, though poorly defined, extending beyond the central bulge. The color profile suggests an older stellar population, dominated by redder hues, particularly in the bulge. There is a subtle gradient in color, with the central region appearing somewhat bluer compared to the outer regions of the bulge and any potential disk structures. Indications of spiral arms or significant dust lanes are absent. There appears to be some minor disturbance to the morphology.