The galaxy appears as a centrally concentrated object with a smooth, diffused morphology. It exhibits a slight elliptical shape, with the major axis subtly elongated relative to the minor axis. A bright core is visible, suggesting a concentration of stars and possibly a central supermassive black hole. The color gradient transitions from a bluer central region to a slightly redder outer halo. No distinct spiral arms or dust lanes are discernible within the resolution of the image. Faint, extended emission is noted surrounding the central body, likely comprised of older stellar populations. There is no evidence of ongoing major merger events. Overall, it seems to be a relatively undisturbed galaxy undergoing moderate levels of star formation.
