The galaxy presents a roughly elliptical morphology, exhibiting a dominant central bulge that appears relatively smooth and concentrated. There is some suggestion of a disk component surrounding the bulge, however, the structure is not well defined. The color profile indicates a yellow/white core possibly transitioning to bluer hues in the outer regions of the disk. There is evidence of some minor disturbances or asymmetries in the outer disk, suggesting a possible interaction or merger event, but it's difficult to confirm. The overall appearance suggests a galaxy with ongoing, but potentially low, levels of star formation activity.
