The galaxy presents as a primarily smooth, elliptical-like structure. The central bulge is bright and concentrated, exhibiting a yellowish-orange hue, suggesting a population of older stars. Fainter, diffuse light extends outwards from the bulge, with a more reddish tint. There is a hint of a disk-like component surrounding the central bulge, though it is not clearly defined. No prominent spiral arms or dust lanes are discernible. The overall shape is generally rounded. There's no clear evidence of ongoing merging activity or major disturbances in the galaxy's morphology.
