The galaxy presents as a somewhat disturbed system, possibly undergoing a merger or interaction. The morphology is elongated and irregular, not exhibiting a well-defined spiral or elliptical structure. There is a suggestion of two distinct nuclei or regions of concentrated light. The overall color is bluish, implying a population of younger, hotter stars. A minor disturbance is apparent; it shows features indicating ongoing or recent star formation activity. There also appears to be some tidal debris or disrupted material extending outward from the main body of the galaxy, supporting the conclusion of an interaction with another galaxy. The estimated size suggests this is not a dwarf galaxy, but a galaxy of moderate size.
