The galaxy presents as a largely smooth, round object with a concentrated central bulge exhibiting a yellowish-orange hue. This is surrounded by what appears to be a disk-like structure. The disk displays a noticeable color gradient transitioning from yellow near the center to a cooler blueish hue around the edges. This implies a possible difference in stellar populations and star formation activity between these regions, with potentially older, redder stars concentrated in the bulge and younger, bluer stars in the disk. There is an indication of a minor disturbance or a possible merging event occurring. An area of distorted light is visible in the lower region of the galaxy, indicating possible gravitational interactions with another object.
