The galaxy presents a largely smooth, elliptical morphology. It exhibits a bright, concentrated core, suggesting a substantial central mass concentration. The light profile appears to fade gradually from the center outwards. The galaxy's overall shape is somewhat elongated, deviating slightly from a perfectly circular form. There appears to be little evidence of significant dust lanes or prominent spiral arm structures. There is a very slight hint of bluer light surrounding the central bulge. There may be slight disturbances within the galaxy's structure, but there are no apparent signs of major mergers or strong tidal interactions with other galaxies.
