The galaxy presents as a moderately luminous object, exhibiting a smooth, elliptical morphology. Its overall color appears slightly redder than the average spiral galaxy, suggestive of an older stellar population. There's a subtle indication of a central bulge which is brighter and more concentrated than the surrounding galactic halo. No distinct spiral arm structures or active star-forming regions are discernible in the image. The galaxy's apparent axial ratio indicates it is observed at a moderate inclination. There are hints of minor disturbances in its structure, possibly related to gravitational interactions. The overall smoothness points towards a galaxy that has undergone significant dynamical relaxation.
