The galaxy presents as a roughly elliptical structure, exhibiting a smooth, concentrated light distribution. The central region displays a higher intensity, indicative of a bright galactic nucleus. The overall color appears yellowish-white, potentially suggesting an older stellar population dominating the light output. There is a subtle color gradient visible, with the outer regions possibly appearing slightly bluer compared to the core, implying some ongoing, albeit potentially subdued, star formation activity in the outskirts. Subtle disturbances in the symmetry of the galaxy's shape could suggest minor gravitational interactions or past merger events. The galaxy displays a moderate angular size.
