The galaxy presents as a spiral type, exhibiting a prominent and elongated central bar structure. The spiral arms are tightly wound around the central bulge. The color suggests a relatively mature stellar population within the core, transitioning to bluer hues along the spiral arms, potentially indicating regions of active star formation. The bulge appears moderate in size relative to the overall galaxy disk, with an elliptical shape. Faint dust lanes are visible within the spiral arms. Based on the slight distortion in the spiral arm structure, it may be undergoing a minor gravitational interaction with a nearby object.
