The observed galaxy presents as a spiral structure with a relatively small angular size. Prominent spiral arms are visible, displaying a somewhat patchy distribution of light, suggesting active star formation regions interspersed with older stellar populations. The color gradient within the arms indicates a range of stellar ages, with bluer regions likely corresponding to younger, hotter stars. The bulge component appears moderate in size, presenting a yellowish-white hue, indicative of an older, more evolved stellar population. There is a suggestion of a faint bar-like structure bisecting the central bulge. Overall, the galaxy appears relatively isolated, with no obvious signs of ongoing major mergers or significant tidal disturbances, although there may be minor disturbances from mergers occurring. The galaxy is seen at a modest redshift, implying a substantial distance. It has a moderate estimated mass and star formation rate.
