The galaxy appears to be a relatively smooth, elliptical-type galaxy. Its core exhibits a concentrated brightness, shifting toward yellow. The outer regions gradually fade into the background, displaying a radial decrease in luminosity. There is no apparent spiral structure or significant dust lanes visible. The overall morphology indicates a galaxy with a relatively old stellar population, with little ongoing star formation. The shape tends to be in between round and cigar shaped. There is no strong evidence of any recent major merging events. A minor disturbance is possible.