The galaxy presents as a relatively smooth, elongated structure. There is a central bulge that appears more concentrated and emits a yellowish-white light, which may indicate an older stellar population. Extending outwards from the central bulge, the galaxy exhibits a flattened disk. The disk shows a somewhat patchy distribution of light. There is a faint bluish tinge to the disk region, which could be indicative of more recent star formation. Overall, the galaxy does not appear to be highly disturbed or interacting with another galaxy. The morphology suggests it is an elliptical galaxy.