The galaxy appears to be a spiral galaxy, viewed nearly edge-on from our perspective. The prominent disk component is oriented approximately vertically in the image. There is a noticeable central bulge that is brighter and more concentrated than the rest of the galaxy. The bulge appears rounded. The disk itself exhibits some degree of lumpy structure, suggestive of star-forming regions or dust lanes, though the resolution limits detailed analysis. Overall, the galaxy appears relatively undisturbed, with no obvious signs of a major merger or significant tidal interaction. There might be minor disturbances.
