The galaxy presents as a relatively small, elliptical object. Its light profile indicates a central bulge, noticeably brighter and more concentrated than the surrounding region. The bulge appears to be composed of older stellar populations, as suggested by its yellowish-white hue. This color contrasts subtly with the slightly bluer, though less prominent, outer regions of the galaxy. The overall morphology appears smooth, with no distinct spiral arm structures or significant dust lanes visible. There is no apparent evidence of ongoing major mergers or tidal interactions with other galaxies. Minor disturbances may be present, however. It appears to be fairly face on and somewhat rounded, though it does appear to be slightly oblong.
