The galaxy presents as a largely smooth, elliptical-like structure with a concentrated central bulge that is the brightest region. There is a slight elongation to the galaxy's overall shape, deviating from perfect circularity. The light distribution suggests a relatively old stellar population throughout, with subtle color variations implying gradients in stellar ages or metallicity. No distinct spiral arms or prominent dust lanes are apparent. There might be a very faint and diffuse disk component, but the image resolution limits a conclusive observation. Overall, the galaxy's morphology is consistent with a passively evolving system, potentially nearing the red sequence.
