The galaxy appears to be a luminous elliptical, exhibiting a generally smooth and concentrated morphology. The central region presents a bright, slightly diffuse core, gradually fading outwards. The galaxy displays a characteristic orange hue, which suggests an older stellar population dominated by evolved red giant stars. There is no clear evidence of spiral arms or a prominent disk structure; rather the overall shape is highly rounded. Subtle irregularities may be present at the very edges of the galaxy, which could indicate minor gravitational disturbances or past interactions with satellite galaxies. However, there is no strong evidence of a major merger in this image.
