The galaxy presents a generally elliptical morphology, appearing somewhat compact and diffuse. The light distribution suggests a central bulge region that is brighter and more concentrated. There are hints of a more extended, fainter halo surrounding the core, particularly in the redder wavelengths. Evidence for spiral arm structures is not apparent.

A portion of the galaxy appears to be disturbed, with a small, somewhat distinct region on one side that exhibits a slightly different color and texture. The morphology suggests there may be an on going minor interaction with another galaxy, or some internal asymmetry or disruption. Otherwise, the overall impression is of a relatively undisturbed, possibly early-type system.
