The galaxy presents a spiral morphology, exhibiting two well-defined spiral arms emanating from a central bulge. These arms are moderately wound and extend outwards, displaying a patchy distribution of light suggesting active star formation regions. The central bulge appears prominent and elongated, potentially indicative of a bar structure. The overall light distribution suggests a relatively face-on orientation, allowing for clear observation of the spiral arm structure. The galaxy exhibits a slight inclination with a moderately high ellipticity.
