The galaxy presents a smooth, elliptical morphology with a high degree of central concentration. The light profile appears largely featureless, with no discernible spiral arms or prominent dust lanes. The color gradient suggests a relatively older stellar population, with a redder hue dominating the central bulge and a subtle blueing towards the outer regions. The galaxy exhibits a noticeable elongation, appearing cigar-shaped, indicating a possible triaxial structure. No significant signs of ongoing merger activity or major tidal disturbances are evident. Overall, the galaxy appears to be a relatively undisturbed, evolved system.
