The galaxy presents as a largely smooth, elliptical structure with a concentrated central bulge. The core exhibits a yellowish-white hue, suggesting an older stellar population with reduced ongoing star formation. The outer regions display a slightly bluer tint, implying some younger, hotter stars, though this is less pronounced than in spiral galaxies. There appears to be a subtle disk-like feature surrounding the central bulge, however the relatively smooth morphology indicates that it is not a spiral galaxy. There is a slight asymmetry to the galaxy's form, with some minor disturbances to the morphology.
