This galaxy exhibits an elliptical morphology with a predominantly smooth light distribution. There is a subtle elongation, but it appears more rounded than cigar-shaped. The galaxy seems to be undergoing a significant interaction, possibly a merger, with another distinct object. This object appears as a separate, though somewhat blended, concentration of light. There are no obviously distinguished features, such as spiral arms or a prominent disk. The color index suggests a relatively older stellar population and limited on-going star formation.
