The galaxy presents a generally smooth, elongated profile, suggestive of an elliptical or lenticular morphology, viewed at an oblique angle. A central bulge, appearing yellowish, is present. Emanating from the central region is a diffuse, bluish envelope. The extent of this envelope indicates a relatively large physical size. There are no clear spiral arm structures, but there appears to be some disruption on the edges that could be signs of tidal distortions. There is possibly another galaxy close to it, so these distortions could be a sign of a galaxy merger event. The light profile suggests a significant stellar mass. The bluish tint in the outer regions may indicate ongoing star formation, though this is not definitively visible.
