The galaxy presents an elongated, disk-like morphology, viewed nearly edge-on. It exhibits a bright, concentrated central bulge or core, which appears slightly yellow to white, suggesting a population of older stars. The galaxy's disk shows a blueish hue, indicative of ongoing star formation. The dust lane is subtly visible and oriented along the galaxy's major axis, obscuring the light from the stars behind it. The galaxy doesn't display any strong signs of interaction or major morphological disturbances, though subtle warping of the disk cannot be ruled out due to the viewing angle. The light distribution follows a Sersic profile that is neither a pure exponential or de Vaucouleurs.
