The galaxy appears as a relatively smooth, elliptical-like structure. Its central region exhibits a high degree of concentration, appearing as a bright, yellowish core, potentially indicating a significant population of older stars. Moving outwards from the center, the color gradually shifts to a slightly bluer hue, suggesting the presence of younger stars in the outer regions, but to a much lesser extent. There's a subtle asymmetry to the galaxy's shape, with a slight extension visible in one direction. There are no prominent spiral arms or dust lanes visible, reinforcing the impression of a galaxy that is primarily spheroidal. The galaxy does not show evidence of a recent major merger, but a minor interaction cannot be ruled out, based on the slight asymmetry. Overall, it presents as a fairly evolved system, consistent with a galaxy that has largely ceased active star formation.
