The galaxy appears to be a single, relatively symmetrical object with a smooth, centrally concentrated light profile. It exhibits a yellowish hue in its core, suggesting an older stellar population. A slight redder tinge is observed in the outskirts of the galaxy, indicating potentially cooler or dustier regions. No prominent spiral arm structures or distinct features are immediately apparent. The overall shape seems largely elliptical, with a high degree of central concentration. The galaxy exhibits minimal signs of tidal interactions or recent major mergers, appearing generally undisturbed. Based on color indices, star formation activity is likely low.
