The galaxy presents as a well-defined spiral structure, exhibiting multiple, prominent arms. These arms appear to be moderately wound. The central bulge is of a moderate size and displays a yellowish hue, suggesting an older stellar population. The disk component of the galaxy shows bluer regions that are indicative of ongoing star formation. There appears to be a faint bar feature. There is no obvious indication of any strong tidal features or significant morphological disturbances, suggesting the absence of any recent major merging events.
