This galaxy presents as a somewhat elliptical structure with a bright, concentrated core. The main body of the galaxy appears relatively smooth with what looks like a slight warp or tilt. Faint blue-ish hues are visible in a ring surrounding the central bulge of the galaxy. These colors could indicate regions of younger stars and ongoing star formation within the disk. There appears to be a disturbance occurring to the right of the central bulge, indicating a possible interaction or merger with a smaller system. The smooth features and lack of strong spiral arms suggest a classification between a spiral and an elliptical, possibly a lenticular or early-type spiral galaxy.
