The observed galaxy exhibits a spiral morphology with a clearly defined disk. Two prominent spiral arms emanate from the central region and trace around the galaxy.

A central bulge is observed, appearing moderately sized and exhibiting a yellowish color, potentially indicating an older stellar population. The disk presents a bluer hue in comparison, possibly indicative of more recent star formation.

There appears to be a bar feature crossing the central bulge of this galaxy. The disk appears to be flocculent, with patchy star forming regions present. The general appearance of the disk indicates the possibility of moderate star formation activity.

There is no obvious signs of tidal streams or other indications of major recent merger events. However, there might be some signs of minor interactions or disturbances, as the arms are a bit disrupted.
