The galaxy appears to be an elliptical type, exhibiting a smooth, concentrated morphology with no discernible spiral arms or distinct features. Its overall shape is largely spheroidal, and it shows high levels of roundness. The central region appears to be brighter and more intensely colored than the outer halo. There may be very mild indications of an interaction with a smaller neighbor, but it's largely isolated. The overall color indices seem consistent with an older stellar population, potentially exhibiting ongoing, but moderate levels of star formation. Its effective radius is around 7 kpc. The estimated mass is around 10^10.8 solar masses. The galaxy is estimated to be at a redshift of approximately 0.26.
