The galaxy appears to be an elongated structure, possibly an elliptical galaxy viewed nearly edge-on, or a spiral galaxy with a prominent bulge and tightly wound spiral arms that are not easily resolved. The light distribution suggests a relatively smooth morphology, although some faint disturbances could be present upon closer inspection. A significant color gradient is observed along the galaxy's major axis, transitioning from blue-ish white at one end to orange-red at the other. This color variation suggests a difference in stellar populations, with the bluer regions likely indicating younger, hotter stars and ongoing star formation, while the redder regions may be dominated by older, cooler stars. There might be a small amount of minor disturbance, but overall the system looks largely undisturbed.
