The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light distribution indicates a system dominated by older stellar populations, emitting predominantly in the redder wavelengths. There is very little indication of any spiral arm structure, or pronounced dust lanes. The morphology suggests the galaxy is an early-type system, likely well past its peak of star formation activity. There is no apparent interaction with nearby galaxies or significant tidal disturbances. The overall appearance is of a galaxy that is relaxed and evolved.
