The galaxy presents as an edge-on disk galaxy. A prominent bulge is visible, appearing smoothly rounded. The disk exhibits an elongated, thin profile, characteristic of edge-on orientations. The light distribution suggests a relatively smooth stellar population within the disk. There is a faint suggestion of dust lanes within the disk, obscuring the light from stars behind them. There is a slight suggestion of minor disturbance in the galaxy's morphology, perhaps indicative of a past or ongoing interaction. Overall, the galaxy appears as a relatively quiescent system with a well-defined structure.
