The galaxy presents as an elliptical morphology, exhibiting a generally smooth light distribution. The galactic core appears bright and concentrated. The object presents a noticeable color gradient, shifting from a bluer hue near the center to a redder tone towards the periphery. This may be due to the distribution of younger, hotter stars towards the center and older, cooler stars in the outer regions, or differential dust extinction. There is no clear evidence of spiral arm structures or a prominent disk. Overall, the galaxy exhibits characteristics consistent with an evolved system.
