The galaxy presents an elliptical morphology, appearing relatively smooth and lacking prominent spiral arm structures. The light distribution indicates a somewhat elongated shape, transitioning from a near-spherical form towards a more cigar-like appearance. The central region exhibits a brighter, more concentrated luminosity profile suggestive of a prominent galactic bulge. There is no apparent major disturbance. Faint hints of bluer colors could suggest a low level of ongoing star formation. Overall, the galaxy appears to be a relatively evolved system with a dominance of older stellar populations.
