This galaxy appears to be a relatively elongated, disk-shaped system seen nearly edge-on. The central bulge is visible, appearing as a concentrated region of yellowish-white light. The disk itself extends outwards from the bulge and is bluer in color than the bulge indicating active star formation. There appears to be some dust or gas obscuring light throughout the disk. No prominent spiral arm structures or bar features are immediately apparent. The galaxy shows only minor signs of disturbance, such as slight tidal tails, and there is no evidence of ongoing mergers or interactions. Based on its color, overall shape, estimated size and star formation rate, this galaxy is most likely a late-type spiral galaxy.
