This galaxy appears to be an elliptical type galaxy, though a disk galaxy may also be possible given the orientation and observed light properties. It exhibits a smooth, centrally concentrated light distribution, indicative of an older stellar population in its core, appearing with a yellow-white hue. Fainter blue regions are slightly more diffuse and more extended from the central core along the major axis, possibly suggesting some ongoing star formation. The galaxy is elongated, with an estimated axis ratio of roughly 2:3. There does not appear to be any major disturbance or merging event, though minor disturbances can not be fully ruled out. The overall structure is relatively undisturbed and symmetric.
