The galaxy presents as a somewhat elliptical, disk-shaped structure, seen nearly edge-on. The central region exhibits a bright, concentrated luminosity, suggesting a significant stellar density or potentially an active galactic nucleus. The disk component shows a distinct blue hue, which is indicative of ongoing star formation. The dust lanes are only faintly present, and appear to show the features of an undisturbed disk. The shape indicates a minor disturbance and there may have been a merger in the distant past.
