The observed galaxy presents as an edge-on spiral galaxy. A prominent central bulge dominates the galaxy's morphology, appearing smooth and with a yellowish-white hue, suggesting an older stellar population. The disk component is visible as a faint, elongated structure extending from the central bulge. There is evidence of a disk, with dust lanes and spiral arms. The disk shows a slight blue color, suggesting the presence of younger stars and star-forming regions. The galaxy exhibits a relatively smooth overall appearance with no signs of a major ongoing merger. There is a possible minor asymmetry or disturbance in the outer disk. The estimated size of the galaxy is approximately 4 kiloparsecs in radius. The galaxy has an estimated mass of 10^11 solar masses. The estimated star formation rate is relatively low.
