The galaxy presents as a yellowish, elliptical-like structure. It has a generally smooth appearance without prominent spiral arms or a distinct central bulge. The distribution of light suggests an oblate spheroidal shape. The color profile indicates a relatively mature stellar population, with the yellower hues being indicative of older, cooler stars. There is a suggestion of a slight tidal disturbance or a minor interaction occurring, but it is difficult to say for sure. There are some slight deviations from symmetry in the outer regions of the galaxy. These asymmetry indicates recent or ongoing interactions. The galaxy is of substantial mass with moderate star formation.
