The galaxy appears as a generally smooth, elliptical-like structure, though not perfectly symmetrical. There is a central bulge with a yellow-white hue, suggesting a population of older stars. Moving outward from the core, the light gradually fades into a bluer tone, hinting at more recent star formation in the outer regions. While the overall shape appears smooth, there are hints of slight disturbances or irregularities in the outer edges, potentially indicating minor gravitational interactions. The overall color profile suggests that star formation activity is present, but not dominant, within the galactic structure. A small fraction of the galaxy's luminosity comes from relatively recently formed, massive stars.
