The galaxy presents a largely smooth and rounded morphology, with a slight elongation. It appears as a single, somewhat diffuse object with a dominant central bulge. Color gradients suggest a possible transition in stellar populations, with a slightly bluer hue around the outer edges. The overall color profile trends towards redder wavelengths, indicative of an older stellar population or significant dust obscuration. There is a subtle hint of asymmetry, which could be due to a minor gravitational interaction or internal dynamics. No distinct spiral arm structures or prominent dust lanes are discernible within the resolution of this image. There is some faint apparent disruption on the lower right side of the galaxy, but the rest of the galaxy has no apparent disturbances. Overall, the galaxy seems to be undergoing a relatively low rate of star formation.
