The galaxy presents as a somewhat elongated, relatively smooth object, with a diffuse, almost hazy appearance. The color profile is dominated by blue hues, indicative of a younger stellar population. There is a slight concentration of light towards the center, which could suggest the presence of a small galactic bulge or a region of heightened star formation activity. The overall structure lacks prominent spiral arms or distinct features, and its uniform luminosity suggests a more quiescent period of star formation. The galaxy shows a minor disk presence, with little signs of an active galactic nucleus, or a recent major merger event. There seems to be no sign of disturbance in the galaxy's form.
