The galaxy presents a primarily smooth morphology with a dominant, concentrated central bulge that exhibits a yellow-orange hue, suggesting an older stellar population. A faint, diffuse disk-like structure extends outwards from the bulge, exhibiting a bluer colouration.  A faint tidal tail-like feature extends outward from the main body of the galaxy, displaying a bluer colour indicating possible star formation. There are minor disturbances in the morphology of the galaxy, potentially indicating tidal interactions or ongoing mergers. The overall shape of the galaxy appears more rounded than elongated.
