The galaxy presents as a centrally concentrated object with a generally smooth morphology. Its core exhibits a bright, yellowish hue, indicating a population of older stars or potentially significant dust obscuration. The isophotes appear largely regular, trending toward elliptical, with no obvious spiral arm structures or prominent star-forming regions discernible. There is a very slight elongation to the morphology, but it is very close to a perfect circle. There is no evident tidal interaction or major merger event disrupting its overall structure, though minor disturbances cannot be ruled out at this resolution. Fainter, bluer regions extend outward from the central bulge, suggesting the presence of a more dispersed stellar population surrounding the core. Given the red shift of this galaxy, and its size, it is a massive galaxy that shows very little to no star formation.
