The galaxy appears to be a spiral type, although the arms are not distinctly defined. There is a suggestion of spiral structure, but it lacks clarity. It is not edge-on. The central bulge is moderately prominent, exhibiting a bright, concentrated region. The overall color is generally pale and somewhat yellowish, which is consistent with older stellar populations. There is a hint of blue in some regions of the disk which indicates some star forming regions are present. There are noticeable disturbances in the overall form; possibly the sign of a merger. There are suggestions of a bar structure across the central region.