The galaxy presents a largely smooth morphology. The light distribution is dominated by a round central region with a bright core. The color is distinctly blue, indicating the presence of a younger stellar population and ongoing star formation, although at a relatively low rate for a galaxy of its estimated mass. There is a slight indication of some minor disturbances or features within the galaxy, but overall it lacks prominent spiral arms or a significant disk component. It appears that the galaxy is not currently undergoing a major merging event, although there may be a very subtle minor interaction.
