The galaxy presents as a centrally concentrated, luminous object with a generally smooth morphology. The overall shape appears roughly circular, exhibiting high degree of symmetry. There is no apparent disk structure or spiral arm presence. Color gradients are subtle, with a slightly bluer hue towards the core transitioning to redder tones in the outer regions. The galaxy's central region is significantly brighter than its surrounding halo, indicating a possible concentration of older stellar populations. There's no apparent ongoing major merger activity or significant tidal disturbances. The faint and diffuse outer regions suggest the presence of an extended stellar halo.
