The galaxy presents an overall smooth morphology, with a slight elongation suggesting a deviation from a perfectly circular shape, appearing somewhat in between round and cigar-shaped. It exhibits a light blue hue, indicative of the presence of young, hot stars and recent star formation. There are no prominent spiral arms or a distinct central bulge visible. No signs of major mergers are apparent. The galaxy appears relatively undisturbed and isolated, with a low probability of any recent or ongoing interaction.
