The observed galaxy presents as a spiral galaxy with a moderate redshift. The galaxy exhibits a prominent central bulge, surrounded by a relatively well-defined disk structure. The spiral arms are distinct, with a morphology indicating primarily tightly wound structures. The color gradient suggests a stellar population distribution with older stars dominating the central bulge, appearing more yellow, and bluer stars populating the spiral arms, though the resolution limits detailed analysis of individual star-forming regions. No significant tidal distortions or signs of recent major merger events are readily apparent. There might be weak bar structure bisecting the central bulge of the galaxy. Overall, the system appears as a relatively undisturbed spiral galaxy undergoing normal evolutionary processes.
