This galaxy appears to be a relatively smooth, elliptical system. Its overall shape is largely round. There is a slight elongation present, but not overtly cigar-shaped. The galaxy displays a concentration of light towards its center, characteristic of a bulge. Moving outward from the center, the light gradually diffuses, indicating a decreasing stellar density.

The central region exhibits a yellowish hue, potentially indicating an older stellar population. The outer regions appear more bluish, perhaps suggestive of some ongoing star formation. There does not appear to be any significant dust lanes or strong spiral arm features. There is no readily apparent evidence of recent major merging events. A slight asymmetry suggests possible minor interactions or disturbances, but the overall morphology suggests a galaxy that has largely settled into a relatively stable configuration.
