The galaxy presents as a relatively faint, elongated structure. The central region exhibits a concentrated brightness, appearing yellowish-white in color. This could be indicative of an older stellar population concentrated in the galactic bulge. Moving outward from the center, the galaxy displays a more diffuse, bluish-white hue. This suggests the presence of a disk with ongoing or recent star formation, contributing to the bluer colors. The galaxy is viewed nearly edge-on, with a high probability of being classified as such based on its morphology. There are faint signs of disturbance but it is unlikely to be undergoing major interaction or merging with another galaxy. The estimated size appears to be moderate, consistent with a spiral galaxy with a substantial disk component.
