The galaxy appears as a relatively faint, flattened disk system seen nearly edge-on. There is a subtle but noticeable bulge at the center, exhibiting a yellowish hue, suggestive of an older stellar population. A thin, bright blueish band stretches across the galaxy's mid-plane, likely indicating active star formation within a prominent dust lane. The overall structure seems largely undisturbed, without significant signs of ongoing major merger activity. The morphology is relatively smooth, with the absence of clearly defined spiral arms. Based on the overall color and morphology, the galaxy is likely a late-type spiral or lenticular galaxy with a relatively high stellar mass and a modest ongoing star formation rate.
