The galaxy presents a dual-component morphology, consisting of a dominant, rounded, smoother feature and a secondary, comparatively blue-shifted, higher surface brightness component. The dominant feature exhibits a smoother texture, suggestive of an elliptical or lenticular morphology. The light is redshifted, indicated by the orange hue. The secondary component appears more compact and of higher surface brightness with a bluer color index, suggestive of ongoing star formation. There appears to be a faint suggestion of some disturbance or irregularity. While primarily round, there is the slightest hint of an elongation. There is a potential sign of a minor disturbance in the galaxy in the form of asymmetry. There might be a sign of a merging event.
