The observed galaxy appears to be a spiral galaxy, exhibiting a prominent disk structure with a central bulge. The spiral arms are clearly visible, showing a morphology predominantly characterized by two arms that appear to be tightly wound. The overall color of the galaxy suggests active star formation, particularly within the spiral arms, indicated by bluer hues. The bulge appears yellowish, likely indicating an older stellar population. There is no apparent bar structure. Morphological indications of ongoing major mergers or significant tidal disturbances are absent, but there is evidence of minor disturbances within the galaxy. The galaxy has an estimated median stellar mass of 10^10.5 solar masses and the galaxy has an estimated median star formation rate of 10^0.2 solar masses per year. This object may be undergoing secular evolution, with a moderate-sized bulge and an active star-forming disk.
