The object appears to be a galaxy at a considerable distance, exhibiting a slightly elliptical morphology. The light distribution suggests a relatively smooth profile, with a concentrated central region. The galaxy shows a color gradient, with a bluer hue at the core, shifting towards redder tones in the outer regions. This color variation may indicate differences in stellar populations or dust content. The smooth appearance implies it is likely an early-type galaxy, although the presence of subtle disturbances cannot be completely ruled out given the image resolution. No clear signs of spiral arms or a distinct disk structure are apparent. The size is relatively compact, suggesting a moderate physical extent.
