The galaxy presents a largely smooth morphology, with a central bulge that appears elliptical in shape. The light distribution suggests the presence of an older stellar population, contributing to the yellow-red hue concentrated in the center. Surrounding the bulge, there is a hint of a faint, disk-like structure, evidenced by a subtle flattening and a slightly bluer color. The disk component appears less prominent, possibly indicating a later-type galaxy with ongoing, albeit moderate, star formation activity. There may be a very small companion galaxy or tidal disturbance at one side of the larger galaxy. Overall, the galaxy's structure leans toward being largely undisturbed.
