The galaxy appears to be an elliptical type, characterized by a smooth, spheroidal morphology. It exhibits a centrally concentrated brightness profile, with luminosity decreasing gradually towards the outer edges. The galaxy's color suggests a predominantly older stellar population, lacking significant blue light indicative of ongoing star formation. There are hints of a slight elongation, deviating from a perfect circular shape. No prominent spiral arms, dust lanes, or active galactic nuclei are discernible. The galaxy appears relatively isolated, lacking obvious signs of major tidal interactions or mergers with other galaxies, although minor disturbances cannot be ruled out. The galaxy's overall appearance suggests it is a relatively evolved and quiescent system.
