The galaxy presents a predominantly smooth morphology. It appears nearly circular, with a slight deviation from perfect sphericity. A concentration of light is visible toward the central region, suggesting the presence of a galactic nucleus. The color gradient transitions from a yellowish core to a bluish-green periphery, which hints at a variance in stellar populations, with older, redder stars likely dominating the center and younger, bluer stars populating the outer regions. There's a hint of some disruption, possibly a minor disturbance, but the overall structure remains largely undisturbed, showing a galaxy in a relatively relaxed state, not currently undergoing major mergers. Based on the color, a low level of star formation may be occurring.
