The galaxy presents a relatively smooth and symmetrical morphology, appearing largely elliptical in shape. The central region exhibits a higher concentration of luminosity, indicating a prominent galactic nucleus or bulge. Progressing outward from the core, the luminosity gradually decreases, forming a diffuse halo. The color distribution suggests a dominant population of older stars, as evidenced by the reddish hue, particularly concentrated towards the core. There are no discernible spiral arms or prominent dust lanes. No signs of major disturbances or ongoing mergers are apparent in the image. The overall appearance points to a quiescent galaxy with minimal recent star formation activity.
