The galaxy appears to be a relatively large, disk-shaped system, seen at a significant angle from edge-on. There is a prominent central bulge that exhibits a yellowish-orange hue, suggestive of an older stellar population. The disk itself appears somewhat patchy, but generally smooth, likely exhibiting a low degree of substructure. The disk also demonstrates a similar yellowish color, with a faint blueish tint at the edges, implying the presence of some ongoing star formation. The overall morphology suggests a classification towards the elliptical side, but with some disk-like components present. The galaxy does not show any obvious signs of major mergers or significant tidal disturbances, but there is a very slight irregular bulge.
