The galaxy presents as a relatively smooth, elliptical form, appearing mostly featureless. Its shape is moderately elongated, displaying a high degree of central concentration. The light is dominated by a bright, yellowish-white core that fades gradually into the outer regions. There is little evidence of spiral arms or distinct substructure within the observed wavelengths. Faint outer regions suggest an extended halo, though the overall boundary of the galaxy is somewhat diffuse and difficult to define with precision. No signs of strong tidal disturbances or ongoing major merger activity are apparent. Subtle color gradients may exist from the core to the outer edges, but further spectral analysis is required to determine the exact nature of its stellar populations and ongoing star formation activity, if any.
