The galaxy presents an elliptical morphology, appearing largely smooth and relatively featureless. It exhibits a concentrated central bulge that graduates outward into a fainter halo. The color profile shifts from a warmer, yellower hue in the core, suggestive of an older stellar population, to a cooler, bluer tone in the outer regions. There is little evidence of spiral arm structure. There is a faint suggestion of a possible minor disturbance or slight asymmetry in its overall form. The galaxy does not appear to be actively merging with another system.
