This galaxy exhibits a moderate redshift, suggesting a considerable distance. Its morphology appears to be predominantly smooth and elliptical in shape. The light distribution indicates a central bulge, with a high concentration of older stellar populations, shown by a yellow and red hue. There is evidence of a slight flattening or elongation, with the general shape of the galaxy more akin to being in between rounded and cigar shaped. Faint blue emission might represent younger stars, however it is not very strong. There appears to be a general lack of substantial ongoing star formation within the galaxy. The overall structure appears largely undisturbed, showing no major signs of interaction or merging events.
