The galaxy presents an overall elliptical morphology. A central bulge is visible, exhibiting a concentrated luminosity gradient with a yellowish hue. Extending from the central region is a disk-like structure that appears somewhat faint and less defined. The disk component shows a subtle gradient in color, transitioning to a bluer tint further from the center. This suggests the potential for ongoing, though likely limited, star formation in the outer regions. There is no evidence of strong spiral arms, but there are some hints of disturbed structures. Given the relative smoothness of the object, it is likely that this object is not undergoing any major mergers.
