The galaxy presents as a relatively small, edge-on spiral system. It exhibits a smooth, elongated profile, with a moderate central bulge that fades into a thin, extended disk. The disk appears to be relatively featureless, lacking prominent dust lanes or spiral arm structures. The light distribution suggests a fairly uniform stellar population throughout the galaxy. The color profile appears relatively blue, potentially indicative of ongoing star formation. No signs of major morphological disturbance or interaction with other galaxies are readily apparent, though there may be some minor asymmetry within the disk suggesting a possible past interaction.
