The galaxy appears as a relatively smooth, elliptical-like structure with a concentrated central bulge. It exhibits a radial gradient in surface brightness, being brightest in the core and gradually fading outwards. The overall color is slightly redder, indicating an older stellar population. There is little to no evidence of spiral arms or distinct dust lanes. No apparent interactions or mergers with other galaxies are visible in this image. The galaxy exhibits a fairly symmetrical, round morphology.
