The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. The central region exhibits a yellowish hue, suggesting an older stellar population. There is a hint of bluer light toward the outer regions, possibly indicating some presence of younger stars, though star formation is either very low or completely absent within the visible spectrum. The overall structure is largely undisturbed, showing no signs of major mergers, though there are a few faint tidal tails or distortions in the halo, potentially suggesting a minor interaction. The galaxy appears fairly compact, and exhibits no prominent disk structure.
