The galaxy presents a morphology indicative of a transition between elliptical and spiral types, possibly a lenticular galaxy. The central bulge is prominent and appears relatively smooth with a yellowish-white hue, suggesting an older stellar population. Diffuse bluer regions extend outward from the central bulge along the major axis, possibly indicative of faint spiral arms with ongoing or recent star formation. These arms are not well-defined. The galaxy's overall shape appears elongated, exhibiting a moderate degree of ellipticity, but is also disturbed. There is evidence of a possible tidal interaction or merger event which causes the galaxy to look disturbed. The outer regions of the galaxy exhibit a faint, diffuse halo.
