The galaxy presents as a disk-shaped structure with a moderately inclined orientation relative to the observer's line of sight. The central region exhibits a bright, concentrated core suggestive of a galactic bulge. The disk shows evidence of spiral arm structures.

The bluer color in the disk likely indicates regions of active star formation. The reddened colors in the central bulge region are indicative of an older stellar population. The overall luminosity suggests a galaxy of moderate mass and ongoing star formation.

There appears to be some evidence of gravitational disturbance, with the disk exhibiting a slightly irregular shape, possibly due to a minor interaction or merger event. The morphology suggests a transitionary phase in its evolutionary history.
