The galaxy presents a predominantly smooth morphology with some indication of disk-like features. Its overall shape approximates a disk.  The central region exhibits a concentrated, high-surface-brightness core.  The galaxy appears flattened, oriented nearly edge-on with respect to the line of sight. Evidence for a dust lane is readily apparent, bisecting the galaxy's central region. Some indications of minor disturbances can be seen within the disk. There is some evidence of possible recent or ongoing star formation activity, judging by the slightly irregular disk.