The galaxy presents a complex morphology, appearing as a system potentially undergoing interaction or exhibiting features indicative of past mergers. The dominant component appears relatively smooth and centrally concentrated with an elliptical morphology. The light from this component exhibits a yellowish-red color, suggesting an older stellar population. A fainter, bluer, disk-like structure is present, viewed edge-on. It connects with the main galaxy, possibly indicating a recent interaction or tidal feature. This disk component exhibits a dust lane. Overall the system is likely a fairly massive galaxy, showing signs of low star formation and a possible recent interaction.
