The galaxy presents as a relatively smooth, elliptical morphology. The light distribution appears centrally concentrated, with a bright, yellowish core. The galaxy exhibits a radial gradient in color, transitioning from the warmer core to cooler, bluish hues in the outer regions. There is a subtle suggestion of a disk component. No pronounced spiral arms or bar structures are readily apparent. Evidence of a recent or ongoing major merger is not evident, although minor disturbances or tidal features cannot be entirely ruled out given the image's resolution. Overall, the galaxy appears to be a mature system with a significant spheroidal component.
