The galaxy presents a largely smooth morphology, appearing elliptical in shape and exhibiting a yellow hue in the observed wavelengths, potentially indicative of an older stellar population. There is very little or no discernable disk structure. The galaxy exhibits a high degree of roundness, closely approaching a spherical shape. There is an additional object close to the galaxy, but without visual evidence of significant tidal disturbance or ongoing merger activity, it is unlikely to be interacting in a major way with it.
