The galaxy appears as a slightly elongated, disk-shaped object. The central bulge is a prominent yellowish-white, suggesting an older stellar population. Moving outward from the bulge, the color shifts slightly to a bluer hue, concentrated in a loosely defined disk. The spiral arm structure is not well-defined, appearing more as a general bluer distribution within the disk. There's a hint of some irregularity or a minor disturbance visible on one side of the galaxy. The galaxy presents a relatively smooth overall appearance, with no strong evidence of a major merger event. It seems to be an intermediate-sized galaxy, with a moderate rate of star formation occurring within its disk.
