The galaxy presents as a somewhat smooth, concentrated light distribution. The central region exhibits a high degree of symmetry and a noticeable yellow hue, suggesting an older stellar population. A slight disc is present, seen close to edge-on, adding some low-level structure. There is also a degree of minor disturbances, possibly resulting from an ongoing interaction or recent merger event. The overall morphology suggests a relatively evolved system that is nearing the final stages of galactic evolution. The apparent lack of strong blue colors or clear spiral arm features indicates a low rate of active star formation.
