The galaxy presents as a slightly elongated, diffuse structure with a dominant, smooth morphology. A faint blue hue permeates the galaxy's body, suggestive of ongoing, albeit modest, star formation activity. The primary body of the galaxy appears to be undergoing some kind of interaction, possibly an earlier minor disturbance, or early stage merger. The is a suggestion of a disk, though this is not fully clear. The galaxy is generally considered to be a intermediate spiral. The observed light distribution suggests a relatively low concentration, indicative of a less evolved system.
