The galaxy presents as an elongated structure, suggesting it is viewed at an angle. The central region exhibits a concentrated, yellowish-white hue, indicative of an older stellar population and potentially a significant bulge component. Fainter bluish extensions are observed emanating from either end of the central region, possibly representing the remnants of spiral arms or tidal features. There appears to be no single dominant arm structure, instead it has an irregular shape. Evidence shows that it may be undergoing only minor interaction with a galaxy. The overall morphology is somewhere between a spiral and elliptical galaxy.
