The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth morphology with a high degree of central concentration. A slight elongation is observed, but it appears mostly round, with a very small probability of being cigar shaped. No prominent spiral arms or distinct disk features are discernible. The galaxy appears relatively undisturbed, with no strong indications of ongoing or recent major mergers. There is a hint of a minor disturbance, but could also be an imaging artifact. The color is a yellowish-orange hue, consistent with an older stellar population and lower star formation rate. Overall, the galaxy seems to be a quiescent system with a smooth, centrally concentrated structure.
