The galaxy presents as a single object with a smooth, elliptical morphology. There is a dominant central bulge with a bright, concentrated core. A fainter, secondary core appears offset from the primary center, perhaps indicative of a recent or ongoing interaction. The light distribution is generally smooth and centrally concentrated with a fairly homogenous yellowish tint. The morphology displays signs of significant disturbances to the stellar disk. Tidal features appear to be present, suggesting possible evidence of merging activity.
