The galaxy appears to be a spiral galaxy, viewed at an oblique angle, with its disk somewhat inclined to our line of sight. There is evidence of spiral arm structure present, although the arms are not sharply defined. The galaxy presents a moderately sized bulge, with a central concentration of light that appears yellowish. The overall color suggests a mix of stellar populations. The disk component shows areas of blueish hues, indicative of younger, hotter stars. There are signs of minor disturbances, possibly due to past interactions or internal dynamics, but no major ongoing mergers are readily apparent.
