The galaxy presents a largely smooth, elliptical morphology. There is a high degree of central concentration, indicated by the bright, nearly uniform luminosity gradient decreasing outwards from the core. No distinct spiral arms or bar structures are discernible. The galaxy exhibits a slightly elongated, nearly circular shape. There is no evidence of significant tidal disturbances or ongoing mergers with other galaxies. Overall, the galaxy appears to be a relatively undisturbed system.
