The galaxy presents as a single, relatively smooth and concentrated light distribution. It appears elliptical in shape, with a high degree of central concentration and a lack of distinct spiral arm features or prominent dust lanes. The galaxy exhibits a yellowish-orange hue, suggestive of an older stellar population and lower levels of ongoing star formation. There is a slight indication of a more extended halo, although the edges of the galaxy fade relatively quickly into the background. The isophotes appear mostly regular, although there may be a very slight asymmetry, precluding any major recent merger events. The galaxy lacks substantial star-forming regions.
