The galaxy presents as a luminous object with a roughly elliptical morphology. The central region exhibits a relatively smooth, concentrated light profile. There is an observed color gradient, shifting from a more yellow-white hue in the nucleus to a redder, slightly fainter periphery. There appears to be a second distinct core of light in the upper portion of the galaxy. The overall structure suggests a possible merging event or strong gravitational interaction, potentially causing the disruption of a typical spiral or elliptical structure. There is a noticeable lack of distinct spiral arms or a well-defined disk.
