The galaxy presents as a centrally concentrated, relatively smooth object. Its morphology appears to be largely spheroidal, exhibiting a gradual decrease in surface brightness from the core outwards. The central region is characterized by a yellowish-white hue, likely indicating a population of older, less massive stars. There is a subtle color gradient toward the outer regions of the galaxy, with hints of a bluer tint that might suggest the presence of some younger stellar populations or ongoing, albeit low-level, star formation. The overall symmetry is slightly perturbed, possibly suggesting minor tidal interactions or disturbances. There is no clear evidence of distinct spiral arms or a well-defined disk component.
