The galaxy presents as a system undergoing apparent interaction, possibly merging, evidenced by the elongated morphology. The primary galactic body appears relatively smooth in texture with a slightly elliptical shape and concentrated central bulge. The color gradient shifts from yellowish-white at the core to a slightly redder hue toward the outer regions. A secondary component is observed to the north of the primary galaxy. This component exhibits a bluer hue, potentially indicative of a younger stellar population or ongoing star formation. There appears to be some distortion in the shape of the primary galaxy, most likely due to gravitational interactions. Overall, the galaxy appears to be in a later stage of its life cycle with suppressed levels of star formation.
