The galaxy presents a somewhat irregular morphology. The central region exhibits a relatively smooth, diffuse appearance, with a dominant yellowish-white hue, suggesting an older stellar population. There is a blue/white region toward the top left and a green/yellow region toward the top right, potentially indicating more recent star formation or different compositions. The galaxy appears somewhat elongated along a vertical axis. There are no discernible spiral arms or a well-defined disk structure immediately visible. Possible tidal features or minor disturbances seem to be present, hinting at past or ongoing gravitational interactions. There is no indication of a strong galactic nucleus.
