The galaxy appears as a lenticular or possibly spiral galaxy, viewed edge-on from our perspective. There is a central bulge that is highly concentrated and bright, with a yellowish hue. This suggests a significant population of older stars residing in the bulge. A flattened disk surrounds the bulge, extending outwards. This disk exhibits some variations in color, transitioning from the yellow of the bulge to a fainter, possibly more reddish hue at the edges. This could indicate the presence of dust lanes within the disk, causing differential extinction of light. There is no indication of recent merger activity or major disturbances in the morphology. There is minimal indication of active star formation. The disk component is relatively smooth in appearance, showing no distinct spiral arm structure at the resolution available.
