The galaxy presents a largely smooth morphology, appearing generally elliptical in shape. It exhibits a high degree of central concentration, with a bright, yellowish core that gradually fades into a less defined, more diffuse halo. The galaxy's color profile suggests an older stellar population dominating its structure, particularly in the core region, indicating a diminished rate of star formation. There is no visible evidence of significant tidal interactions or major mergers, and no clear spiral arm structures are apparent. Overall, the galaxy appears to be a relatively undisturbed, mature system.
