The galaxy presents as a singular, though visibly disturbed, system. It is observed to have a predominantly smooth morphology, with the overall light distribution appearing diffuse and centrally concentrated. The shape is generally rounded, though not perfectly spherical, with a slight elongation evident. There is evidence of a minor disturbance, possibly due to a past or ongoing interaction.

A secondary, smaller concentration of light is seen offset from the main body. This could potentially represent a tidal dwarf galaxy that is undergoing a merger with the primary galaxy. It is hard to say for certain based on the image.

The color is consistent across the primary and secondary concentration of light, which may hint that there is a lack of on-going star formation.