The galaxy appears as a slightly elongated, relatively smooth structure. It presents a yellowish-white central region, potentially indicating an older stellar population or significant dust obscuration. The overall form suggests an intermediate stage between elliptical and disk galaxies. There is a hint of a disk-like component but no clear spiral arm structure.

The galaxy exhibits a subtle asymmetry, possibly due to tidal interactions or minor mergers in its past. No prominent dust lanes or star-forming regions are immediately apparent. The apparent smoothness of the galaxy suggests a significant fraction of its light is emitted from an older stellar population.
