The galaxy presents as a smooth, elliptical-like structure with a central bulge. The light distribution appears relatively even, lacking significant spiral arm features or prominent dust lanes. The galaxy's color profile suggests an older stellar population, with a yellowish-white hue dominating the central region, potentially indicating a higher concentration of evolved stars. The outer regions exhibit a slightly bluer tint, which may suggest ongoing, but diminished, star formation compared to the central region. Overall, the galaxy appears undisturbed, showing no obvious signs of a recent major merger or interaction.
