The galaxy presents as a single, somewhat diffuse object with a relatively smooth light profile. It appears approximately round, with a subtle elongation. There's a color gradient visible, transitioning from a more yellowish-orange core to a slightly bluer outer region. This color gradient suggests a possible variation in stellar populations, with older stars concentrated toward the center and younger, bluer stars more prevalent in the outer regions. While the object appears largely undisturbed, there might be some slight asymmetry suggesting past or ongoing gravitational interactions, but further analysis is needed to confirm.
