The galaxy presents as a relatively smooth, disk-shaped structure. Its color profile exhibits a slight central concentration with yellowish hues, transitioning to a fainter, bluer outer region. The galaxy appears slightly elongated with an inclination relative to our line of sight. There is no evident presence of spiral arm structures or strong dust lane obscuration. The overall morphology suggests a galaxy that may be undergoing, or have undergone, a transition in its star formation activity, with some ongoing activity, but not extremely significant. The smoothness indicates the lack of recent major merger events and potentially the absence of a dynamically young stellar population throughout a significant portion of the galaxy.
