The galaxy appears to be elliptical in shape, with a high degree of central concentration. The light profile is smooth, lacking prominent spiral arms or other distinct features typically associated with disk galaxies. The dominant color is yellow-orange, suggesting an older stellar population with relatively little ongoing star formation. There is an apparent faint nucleus which is highly unresolved. There are no obvious signs of interaction or recent merger activity, although there may be some very slight disturbance in its overall structure.
