The galaxy presents as a disk galaxy, likely an early-type spiral or lenticular, observed at an oblique angle relative to our line of sight. The central bulge is prominent and exhibits a yellowish-white hue, possibly indicating an older stellar population. The disk component appears relatively smooth with a bluer color, hinting at ongoing star formation. There is a minor disturbance in the structure. The galaxy displays an elongated shape, suggesting it is not perfectly face-on. No distinct spiral arm structure is readily apparent.