The galaxy presents a relatively smooth, elliptical morphology, appearing largely featureless in the available image. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards its outer regions. The color profile indicates a presence of older stellar populations. The galaxy is likely a spheroid system with no apparent spiral arm structures. The object's slight elongation suggests a minor degree of flattening, but its overall shape is predominantly round. Faint traces of blue light may indicate subtle star formation in its periphery, however, the galaxy is composed largely of older stars. The galaxy does not display any signs of major disturbances or ongoing mergers with other systems.
