The galaxy presents an overall elliptical morphology, appearing as a flattened spheroid. A bright, concentrated central bulge dominates the galaxy's core, exhibiting a yellowish hue indicative of an older stellar population. The outer regions display a fainter, more diffuse disk-like structure, with hints of reddish tones, suggesting a mix of older stars and dust. The galaxy's edges are somewhat ill-defined, fading gradually into the background. There is a subtle asymmetry in the outer regions, potentially due to tidal interactions or internal disturbances, though no distinct merger features are immediately apparent. The relative smoothness of the light distribution implies a relatively relaxed dynamical state, with a moderate degree of ongoing star formation in localized regions.
