The galaxy presents as a faint, elongated object, likely a spiral galaxy viewed at a high inclination. It appears cigar-shaped. The central bulge is subtly visible and displays a yellowish hue, suggesting an older stellar population. Fainter bluish regions are observed extending from the bulge, tracing the spiral arms. These regions may indicate areas of more recent star formation. There is what appears to be a bright knot of emission, suggesting the presence of an HII region or possible tidal disturbance, on either side of the main galactic body. The overall structure seems relatively undisturbed, implying the absence of a recent major merger event. The galaxy exhibits a moderate redshift, indicating that the light has traveled a significant distance and provides information about the galaxy's velocity relative to Earth. Given its apparent magnitude, the estimated size and luminosity suggest it is a galaxy of moderate mass. The color indices indicate a relatively normal stellar population for a galaxy at this redshift.
