The galaxy exhibits an elliptical morphology with a smooth light distribution, showing minimal discernible features like spiral arms or distinct dust lanes. The galaxy's color profile suggests an older stellar population, with a central bulge that appears more luminous and exhibits a slightly redder hue, which could indicate a higher concentration of older, redder stars. The outer regions fade into a bluer tint, possibly due to more recent star formation at the galactic edges or an abundance of younger, bluer stars. Overall, it is an elliptical galaxy, likely a few kiloparsecs across, with a moderately flattened shape and consistent color gradients between the bulge and outer regions.
