The galaxy presents as a relatively smooth and centrally concentrated object. It has an elliptical morphology, appearing nearly circular with a slight elongation. The light distribution is dominated by a central bulge, characterized by a bright, diffuse glow. The outer regions of the galaxy exhibit a gradual decrease in surface brightness, fading into the background. There is no readily discernible spiral structure or prominent dust lanes within the visible extent of the galaxy. The overall color appears to be slightly redder, suggesting a population of older stars.
