The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge which emits a yellow-white light, likely composed of older stellar populations. The galaxy presents a highly rounded morphology, showing no obvious disk features or signs of a recent major merger. There might be very faint and diffuse outer regions with redder hues extending beyond the main body, though these are not well-defined in the available imaging. Overall, the galaxy seems quiescent, with low rates of star formation.
