The galaxy presents as a generally smooth object, appearing largely elliptical in shape. There is a discernible, bright central bulge that seems nearly spherical, exhibiting a yellowish hue. The outer regions diffuse outwards from this core, showing a bluer color profile, suggesting the potential presence of a stellar disk component with relatively recent star formation activity. The overall structure lacks strong spiral arms or other features denoting a highly structured morphology, but there are some subtle disturbances that may suggest past merger activity. The galaxy's light distribution appears relatively even, with a smooth gradient from the core outwards. The galaxy has a relatively high mass and relatively low star formation rate.
