The galaxy presents as a largely elliptical structure with a smooth, centrally concentrated light distribution, suggesting a dominant spheroidal component. There is a slight elongation, deviating from a perfectly circular shape, with only very minor potential disturbances. The galaxy's color profile is characterized by a generally redder central region gradually transitioning to bluer hues in the outer regions. The overall color suggests an older stellar population residing within the inner region, while more active star formation may be present in the outer parts. The galaxy's size suggests that this may be a large galaxy.
