The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a concentrated brightness, appearing a yellowish-orange hue. Progressing outward, a subtle transition to a bluish halo is observed, extending somewhat beyond the core. The overall shape is elongated, with the long axis oriented horizontally in the image frame. There are no discernible spiral arms or distinct dust lanes visible; the light distribution appears relatively uniform across the galaxy's body. The color gradient suggests potential variations in stellar populations, with the core possibly dominated by older, redder stars, and the outer regions exhibiting a component of younger, bluer stars. The galaxy does not appear to be undergoing any major merger events, though very subtle disturbances cannot be ruled out at this resolution.
