The galaxy appears as a somewhat elliptical, centrally concentrated system. Its overall light distribution is smooth, with no readily discernible spiral arms or other complex structures. The color gradient shifts from a yellow-white core to a redder, more diffuse outer halo. The lack of sharp features suggests a relatively old stellar population and a low ongoing star formation rate. Evidence of recent or ongoing merging activity appears to be negligible, and the galaxy exhibits a generally undisturbed morphology. The estimated size of the galaxy is several kiloparsecs. Based on its morphology, color, and lack of discernible features, this galaxy is likely an elliptical.
