The galaxy presents a complex morphology, appearing to be an interacting system. A prominent, relatively smooth and rounded central component dominates the structure. This component exhibits a slight elongation and color variation; the color is slightly more green and yellow than blue. A diffuse, less luminous feature extends from this central component, showing a lower surface brightness and a bluer overall color, indicative of younger stellar populations. This extended feature suggests a tidal interaction or a merging event.

The lack of clearly defined spiral arms in the primary structure suggests the system is either an elliptical galaxy undergoing a tidal interaction, or a spiral galaxy heavily disrupted by a recent merger. The relative sizes and luminosities of the two components indicate a possible major merger event. The overall structure exhibits signs of disturbance, ruling out a classification as a regular elliptical galaxy. Further spectroscopic analysis would be required to determine the redshift, stellar populations, and gas content to better characterize the nature of this system and the ongoing interaction.
