The galaxy presents as a spiral type, observed at an oblique angle, approaching edge-on. It is composed of a distinct, bright central bulge with a yellowish hue. This bulge appears relatively smooth, suggesting an older stellar population and potentially a supermassive black hole at its center. A relatively faint and slightly more blueish disc surrounds the bulge, indicating the presence of ongoing star formation.

Dust lanes are visible as dark, patchy regions within the disc. These lanes are concentrated in the equatorial plane of the galaxy. There are no obvious signs of a major ongoing merger event, though there could be signs of minor tidal disturbances or interactions. The disk structure appears somewhat flocculent, lacking grand, well-defined spiral arms. Overall, the galaxy exhibits characteristics consistent with a late-type spiral galaxy, with moderate star formation activity and a relatively well-defined morphology.
