This galaxy appears to be a spiral galaxy, observed at an oblique angle. It exhibits a central bulge that is significantly brighter than the surrounding disk. There appears to be a disk, which is noticeably flattened, with a dust lane or obscuration visible along the equatorial plane, although it is not sharply defined. The spiral arms are subtle, and the galaxy's overall color suggests an older stellar population, with a lower rate of ongoing star formation. Overall, the galaxy presents as a relatively well-ordered spiral structure, showing characteristics of a later-type galaxy. There are no prominent signs of recent mergers or tidal disturbances.
