The galaxy exhibits a flattened, elongated morphology, appearing as a disk galaxy observed at a significant inclination relative to our line of sight. The central bulge is prominent, displaying a concentrated, yellowish-white luminosity suggestive of an older stellar population. Moving outwards from the bulge, the disk reveals a mixture of colors, with regions of bluer light indicative of ongoing star formation and younger stellar populations. Dust lanes appear subtly within the disk, contributing to the galaxy's somewhat irregular structure. The disk edges are diffuse. The galaxy appears to be undergoing some type of disturbance as the morphology is not even, and there appears to be a tidal tail.
