The galaxy presents a notable disk structure with prominent spiral arms. The arms appear relatively tightly wound, emanating from a central bulge. The bulge itself is moderately sized and exhibits a yellowish hue, suggestive of an older stellar population. A bar-like structure seems to traverse the central region, further influencing the spiral arm morphology. The disk is not perfectly edge-on; a clear inclination allows for the observation of spiral features. The spiral arms show a mix of bluer and redder regions, implying a combination of recent star formation and older stellar populations within the arms. There are no obvious signs of major mergers or significant tidal disturbances affecting the galaxy’s overall structure.
