The galaxy presents as a centrally concentrated object with a smooth overall appearance. The light distribution is dominated by a central bulge that appears almost spheroidal. There is a slight elongation noticeable along one axis, but it is not a strongly barred spiral. The color is generally whitish, indicating the presence of an older stellar population. Faint, blue-tinged extensions are visible at the edges of the galaxy, these are suggestive of on-going, low levels of star formation. There is no clear evidence of spiral arms or significant dust lanes. There are no signs of a major merger event, although the slight asymmetry of the light profile suggests it might be experiencing minor interactions.
