The galaxy presents a generally smooth, elliptical morphology, appearing largely featureless. The light profile suggests a centrally concentrated bulge. Coloration indicates the presence of a dominant older stellar population, emitting primarily in the redder wavelengths, with a yellowish hue toward the center, possibly indicating a concentration of older, cooler stars. There is a slight bluer tint on the edges. There is no clear evidence of spiral arms or a distinct disk structure. The overall appearance suggests a system that has largely ceased active star formation. The roundness of the galaxy suggests that we are viewing it from a roughly face-on perspective. There are no major visible signs of tidal disturbances or interactions with other galaxies, although minor disturbances cannot be entirely ruled out given the limitations of the image resolution.
