The galaxy presents an elliptical morphology, appearing predominantly smooth with no readily discernible spiral arm structure. The color gradient transitions from a bright, yellowish-white core, suggestive of an older stellar population, to a redder and less intense halo. The apparent elongation indicates a non-spherical shape, leaning towards a cigar-like appearance but generally more oval. There is no obvious evidence of active galactic nuclei activity or significant dust lanes. The overall structure appears relatively undisturbed, lacking strong signs of recent or ongoing major mergers. Faint hints of asymmetry are present in the outer regions, but no substantial tidal features are observed.
