This galaxy presents a moderately elliptical morphology. Its core appears bright and concentrated with a yellowish hue, suggesting a population of older stars. Surrounding the core, there is a less concentrated and bluer halo, indicating the presence of younger stars or ongoing star formation. The galaxy doesn't exhibit any clear spiral arm structure. There may be some minor disturbances visible in the galaxy’s shape, but the main body appears relatively smooth. The galaxy exhibits an intermediate level of roundness, between perfectly spherical and elongated. Overall, the galaxy seems to be in a relatively stable state, without any signs of a recent major merger.
