The galaxy presents as a disk galaxy with a relatively smooth, moderately concentrated bulge. The galactic disk appears tilted, presenting an elliptical profile. The bulge exhibits a brighter, yellowish hue indicative of an older stellar population. The disk shows a bluer coloration, suggesting the presence of younger, hotter stars, perhaps indicative of ongoing star formation. There are disturbances, either from a minor collision or an artifact in the image. There may be a possible central bar feature, although this is difficult to discern definitively from the image.
