The galaxy presents a generally smooth and elliptical morphology. Its light is concentrated towards the center with a bright, compact core, implying a significant bulge component. The outer regions exhibit a more diffuse glow, gradually fading into the background sky. There is very little evidence of spiral arms or significant dust lanes, suggesting it is likely an early-type galaxy. The lack of blue light indicates a population of older stars. No obvious signs of tidal disturbances or interactions with other galaxies are visible in this image.
