The galaxy presents as a slightly elongated structure. There appears to be a central bulge that is brighter and more concentrated than the outer regions. It is difficult to ascertain from the image alone whether this is a true elliptical or a spiral galaxy viewed edge-on, however there are hints of a disk extending from the central region. The disk seems somewhat disturbed or patchy. The galaxy exhibits a bluish hue, suggesting the presence of some younger, hotter stars. There are no distinct spiral arms visible, indicating that if it is a spiral galaxy, the arms are either tightly wound or obscured by dust. The overall morphology appears to be relatively smooth, but with hints of internal structure.
