The observed galaxy presents as a disk galaxy, viewed nearly edge-on from our vantage point. The disk appears relatively smooth and featureless, lacking prominent spiral arm structures or significant dust lanes. The central bulge region is notable for its enhanced luminosity and a yellowish hue, suggesting an older stellar population. The outer regions of the disk exhibit a bluer color, indicative of ongoing star formation. The galaxy shows no obvious signs of major disturbances or mergers. Faint asymmetric tidal features may be present, but further investigation is required. The galaxy exhibits a moderate redshift, suggesting a considerable distance from the observer. Overall, the galaxy appears as a relatively undisturbed, moderately massive system undergoing moderate levels of star formation.
