The galaxy appears to be a relatively smooth, elliptical system with a concentrated central bulge. Its overall color is yellowish, possibly indicating an older stellar population with a reduced rate of star formation. The morphology suggests the galaxy is transitioning towards a more passive state. There may be a slight visual elongation present, although it is mostly round. There's little evidence of spiral arms or major mergers and distortions. The lack of significant blue regions or obvious dust lanes further supports the assessment of a relatively quiescent galaxy.
