The galaxy presents as a relatively compact object with a centrally concentrated luminosity profile. The overall morphology appears to be smooth and elliptical, lacking any prominent spiral arms or bar structures. The core region exhibits a bright, yellowish-white color, which could indicate an older stellar population. Surrounding the core, the galaxy displays a slightly bluer hue, potentially suggesting more recent star formation activity in the outer regions. There is a subtle hint of asymmetry or minor disturbances in the galaxy's outer structure, possibly resulting from past interactions or mergers. The shape of the galaxy appears to be somewhere in between round and elliptical. Overall, the galaxy appears to be a relatively massive system with ongoing, albeit possibly subdued, star formation.
