The galaxy appears to be a disk galaxy, viewed at a relatively high inclination. Its shape is generally smooth and the light distribution suggests a significant bulge component. There may be evidence of weak spiral arm structure, although the arms are not well-defined. The color of the galaxy is relatively uniform across its surface, with a slightly more yellow or orange hue, which might indicate an older stellar population and lower star formation rate. The galaxy's relatively smooth appearance and color point to it being an early-type spiral or possibly a lenticular galaxy. There may be a fainter galaxy close in proximity, although it could also be a star.
