The galaxy presents as a relatively smooth, rounded structure. A bright central bulge is visible, exhibiting a yellowish hue, suggesting a population of older stars. The outer regions of the galaxy display a more bluish tint, potentially indicating ongoing star formation. There is a slight hint of a disk structure, but overall the morphology appears mostly spheroidal. There are possible indications of minor disturbances or tidal features, though not distinctly defined. No clear evidence of a major merger is apparent. The galaxy is generally compact in appearance.
