The galaxy presents as an elliptical system, exhibiting a smooth, relatively featureless morphology. The central region displays a bright, concentrated luminosity, gradually decreasing towards the outer edges. There is a slight elongation, suggesting it is not perfectly spherical but instead is more "in between" on a roundness scale. A possible tidal feature exists that may suggest an interaction. The overall color is consistent with an older stellar population, with a yellow-red hue dominating, but there is evidence of star formation. The mass of this galaxy is estimated to be between roughly 9 and 10 to the power of 9. The rate of star formation is estimated to be roughly between 10 to the power of -5 and 10 to the power of -2 solar masses per year. 
