The galaxy presents a predominantly smooth and rounded morphology, with a slight elongation. Its color profile indicates a concentration of older stellar populations, exhibiting a yellowish hue at its core, which transitions gradually towards a redder color in its outer regions. There is no strong evidence of distinct spiral arm structures or active star formation regions visible in this image. Based on the color distribution and shape, this galaxy is likely an elliptical galaxy, showing no significant signs of ongoing major mergers, though minor disturbances cannot be ruled out.
