The galaxy appears as a somewhat elongated, yellowish-orange structure. The central region exhibits a brighter, more concentrated luminosity, suggesting the presence of a significant bulge component. The overall morphology is generally smooth, with no prominent spiral arms or distinct dust lanes visible in this image.

The galaxy displays a noticeable color gradient, with the central region appearing more yellow, possibly indicating an older stellar population. The outer regions seem to have a slightly bluer hue. The galaxy shows no strong signs of a major ongoing merger, though there may be some minor asymmetry or disturbance present within the outskirts.
