The galaxy presents as a disturbed system, likely undergoing a merger or interaction. It exhibits an irregular morphology with an estimated effective radius of approximately 4.5 kpc. There are at least two distinct nuclei visible within the galaxy. A luminous tidal tail or bridge is apparent, connecting the two core components. This is suggestive of ongoing gravitational interaction. The galaxy has a moderate luminosity and a redder color profile, indicating that it is composed of an older stellar population with a low specific star formation rate. The overall shape appears somewhat elongated but not distinctly barred or spiral in nature.
