The galaxy presents as a luminous, centrally concentrated structure. Its morphology suggests a disk galaxy, viewed at an oblique angle. The galaxy exhibits a relatively smooth, but detailed appearance. The central bulge appears prominent and bright, gradually fading into a disk. Star formation appears to be present within the galaxy. There are no signs of tidal tails, strong gravitational disturbances, or other clear indicators of an ongoing major merger event. It is likely that this galaxy is in a relatively stable state.
