The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape is elliptical, with a high degree of roundness. The galaxy exhibits a color gradient, transitioning from a yellowish-orange core to a bluer outer region. This color variation suggests older stellar populations dominate the central bulge, while younger, star-forming regions are more prevalent in the outskirts. A faint, asymmetric extension is visible on one side, possibly indicating a minor tidal interaction or disturbance. There is no obvious evidence of spiral arms or a prominent disk structure.
