This galaxy presents as a relatively smooth, elliptical structure. The color profile exhibits a dominant yellowish hue, suggestive of an older stellar population. The galaxy appears generally spheroidal, with a high degree of central concentration of light. There is little evidence of spiral arms or prominent dust lanes. There may be a faint, diffuse halo surrounding the central core, although this is difficult to ascertain with certainty. The overall morphology is consistent with an early-type galaxy with moderate mass. There is no clear indication of a major ongoing merger event, though minor disturbances cannot be entirely ruled out.
