The galaxy presents a clear spiral structure, exhibiting two prominent arms extending from a central bulge. The arms appear loosely wound. The bulge itself is moderately sized and displays a yellowish hue, suggesting an older stellar population. The spiral arms are bluer in color, potentially indicative of ongoing star formation. A weak bar structure seems to transect the central bulge. There are no obvious signs of major mergers or significant tidal disturbances. A region of increased redness is seen in one of the arms, suggestive of dust obscuration or localized older stellar populations. Overall, the galaxy appears to be a relatively undisturbed spiral galaxy undergoing moderate star formation.
