The galaxy presents as a disk galaxy, though the inclination obscures a clear face-on view. The disk exhibits a noticeable blue hue, especially in several distinct regions, suggesting ongoing star formation. The distribution of this blue light hints at the presence of spiral arm structures, though they are somewhat ill-defined. The central region appears more amorphous. There is no clear central bulge, but the central mass distribution is difficult to determine due to the lack of clear definition and moderate inclination. The overall shape is somewhat irregular, potentially indicating a minor gravitational disturbance or past merger event. The light emitted suggests a relatively low rate of star formation. There is no clear bar structure visible. The morphology of the galaxy is therefore suggestive of a late-type spiral or irregular galaxy undergoing mild evolutionary activity.
