The galaxy presents as a generally smooth, elongated structure. Its central region appears significantly brighter and more concentrated, exhibiting a yellowish-white hue, suggestive of an older stellar population. Surrounding this core is a fainter, bluish-white disk, which may indicate the presence of younger stars. The galaxy lacks any prominent spiral arm structure. The overall morphology indicates this may be an elliptical galaxy or a lenticular galaxy viewed edge-on. There are no obvious signs of tidal disturbances or ongoing mergers.
