The galaxy presents a somewhat smooth morphology, appearing largely spheroidal in shape, with an apparent high degree of roundness. There is a hint of some structure, perhaps a very faint disk-like feature, but this is not prominent. The galaxy exhibits a moderate red shift, with a spectral distribution peaking in the R band, indicative of an older stellar population. The absolute magnitude of the galaxy is relatively high, suggesting it is a luminous object. There is the suggestion of a minor gravitational disturbance event or possible merger occurring. However, this is uncertain. The light is evenly distributed from the center, no blue regions are observed.