The galaxy presents as a generally smooth, elliptical structure. Its overall shape is elongated, appearing somewhat cigar-shaped. The central bulge appears to be relatively bright and dominates the galaxy's luminosity profile. There is a faint disk surrounding the central bulge. The color is slightly reddish, suggesting a population of older stars. There is no clear evidence of distinct spiral arms or active star formation regions, although there may be a very low level of star formation. The galaxy does not show obvious signs of a major merger event, though a minor disturbance cannot be ruled out.
