The galaxy presents a generally smooth, elliptical morphology. It appears to be relatively luminous, with a bright, concentrated central bulge that gradually fades into a less dense, extended halo. The color distribution is somewhat uniform, showing a yellowish-white hue at the core, suggesting an older stellar population. There's no prominent evidence of spiral arms or significant dust lanes. There is a subtle color variation in the outer regions, showing some faint blue light. No major disturbances or signs of ongoing merger events are immediately apparent in the galaxy's structure. The overall appearance points toward a galaxy with a substantial mass and relatively low star formation rate compared to its mass.
