The galaxy presents as a single, centrally concentrated object with a relatively smooth light distribution. It exhibits a generally elliptical morphology, appearing mostly round with only slight elongation. The galaxy's color is predominantly yellowish-orange, suggestive of an older stellar population and relatively low ongoing star formation. There appear to be some minor disturbances and signs of interaction, possibly a very early stage merger, given the slight irregularities in its overall form. The galaxy's considerable size suggests a large stellar mass.
