The galaxy presents as a relatively smooth and centrally concentrated system. Its overall shape is somewhat elongated. There is a clear, bright central region indicative of a substantial galactic nucleus, which is slightly yellow in appearance. The galaxy's body displays a color gradient, shifting from a yellowish center to bluer edges. This suggests active star formation or a population of younger, hotter stars in the outer regions. While the galaxy exhibits a predominantly undisturbed morphology, subtle asymmetries may indicate minor gravitational interactions or past merger events. The light distribution falls off gradually towards the edges, showing no distinct spiral arms or bar structures.
