The galaxy presents an oval morphology, appearing somewhat amorphous in structure. The light distribution suggests a central concentration, though it is not sharply defined. Faint, diffuse extensions are visible, hinting at possible tidal interactions or past minor merger events. The color profile appears relatively uniform, displaying a subtly bluer hue overall. No distinct spiral arms or a prominent central bulge are apparent, though some small, amorphous regions of blue suggest areas of on-going star formation. The galaxy may have experienced some past gravitational disturbances but is largely relaxed.
