The galaxy presents a generally smooth appearance with some subtle features. It exhibits a flattened, disk-like structure oriented close to edge-on with respect to our line of sight. A bright central bulge is observed, surrounded by a relatively faint, extended halo. The halo displays a subtle greenish coloration possibly indicative of emission lines. Evidence of a faint dust lane is observed, bisecting the bulge and disk, appearing as a darker region. No spiral arm structures are definitively detected. Minor disturbances may be present within the disk. Overall, the galaxy is relatively undisturbed, without any major mergers ongoing.
