The galaxy presents a generally smooth morphology, with a concentrated central region. It exhibits a flattened, disk-like structure, viewed at an oblique angle. There is an indication of asymmetry, potentially due to a minor gravitational interaction or internal activity. The galaxy's color gradient suggests a slightly older stellar population dominating the central bulge, transitioning towards bluer hues in the outer regions of the disk. No prominent spiral arm structures are readily discernible, possibly due to limitations in image resolution or the galaxy's intrinsic characteristics.
