The galaxy presents as a relatively smooth, centrally concentrated object. Its overall form appears elliptical or possibly a tightly wound spiral, although definitive spiral arms are not discernible in this image. The central region is characterized by a bright, yellowish hue, suggesting a population of older stars and potentially a significant bulge component. Moving outwards from the core, the color transitions to a slightly bluer tint, possibly indicating the presence of younger stars or ongoing star formation, albeit at a modest rate. The galaxy exhibits a high degree of radial symmetry, with only subtle deviations from a perfectly elliptical shape. There is no clear evidence of major mergers or significant tidal disturbances. The lack of obvious dust lanes further supports the classification of this galaxy as an early-type spiral galaxy. The apparent magnitude suggests that it has a substantial stellar mass. Overall, it is a large, isolated galaxy.
