The galaxy appears to be a relatively smooth, elliptical type. It exhibits a concentrated central bulge that transitions gradually into a more diffuse outer region. The color profile is generally yellow, suggesting an older stellar population with less ongoing star formation, however, there is evidence of bluer regions within the halo of the galaxy. It appears relatively undisturbed, showing no signs of significant tidal interactions or major mergers. There is a slight asymmetry to the galaxy, possibly indicative of a minor disturbance or past interaction. It is approximately circular in shape with a slight elongation.
