The galaxy appears to be a spiral galaxy, viewed at a slight angle relative to edge-on. Evidence of spiral arm structures is visible, though they are not sharply defined. The central bulge appears prominent and moderately sized, displaying a smooth, concentrated distribution of light. The disk exhibits a less smooth texture, with hints of patchy regions that may correspond to star-forming regions. There is no apparent bar feature bisecting the bulge. The galaxy appears relatively isolated, showing no obvious signs of ongoing major merger activity, though minor tidal disturbances or interactions cannot be ruled out based solely on this image.
